The Pedra Branca massif is located in central Brazil, northeast Goiás, near the city of Nova Roma, occupying an area of approximately 80 km2. It is part of the Goiás Tin Province (GTP), located within the oldest tin subprovince, Rio Paranã, which, together with the Rio Tocantins Subprovince, are the most economically important provinces of the GTP. The massif is part of the Pedra Branca suite and is defined as an A-type granite from the Paleoproterozoic (1.6–1.77 Ga), rich in several ores such as tin, fluorine and rare-earth elements (REE) with anomalous concentration of indium, niobium, uranium, and thorium. Its magmatic evolution is closely related to the continental evolution and bimodal volcanism of the Araí rift. The mineralization zones are pre-tectonic, hosted in greisens with the presence of cassiterite; the main mineralization zones are named Zona da Bacia and Faixa Placha. This area is characterized by metallogenic importance. However, only a few geophysical studies have focused on the granite area. The lack of geophysical information makes it difficult to establish the signature of the Pedra Branca massif. The main goal of this study is to increase geophysical information by determining the magnetic and gamma-ray spectrometric signatures of the granite massif, and to generate a geophysical-geological model representative of the surface and subsurface geological features. These signatures are investigated and related to the geological structures and tin mineralized zones (cassiterite) present in the massif. Based on the analysis of airborne and ground gamma-ray spectrometry data and geochemical data, it was possible to characterize the anomalous zones of uranium (U) and thorium (Th) of the granitic massif. From the magnetometric Total Gradient Amplitude (TGA) and Tilt Derivative (TDR) products, it was possible to define important magnetic signatures, as well as to delimit the intrusion and its contact with enclosing and surrounding rocks. These products, in conjunction with products generated by Matched Filtering and Euler Solutions, provide subsurface magnetic signature information and their depth estimates. The forward modeling and the inversion of the magnetic data generated from the Induced Magnetization Vector (MVI), were correlated in order to generate a 2D geophysical-geological model that presents main sources of shallow magnetic susceptibility (ca. 800 m) corresponding to the Faixa Placha (0.029SI) and sources of high susceptibility (0.012SI - MVI), located in greater depth (ca. 2 km) inside and outside the massif. Within the massif, the source of high susceptibility was interpreted as mafic pluton due to the bimodal magmatism of the Araí rift. On the surface, this mafic magmatism emerges as diabase dikes. The other magnetic source in the southeast edge is interpreted like a mafic magmatism body from the bimodal volcanism of Araí Group or Quartz Diorite Nova Roma. The interpretation of geophysical data is consistent with the underplating process, commonly accepted as responsible for the generation of type A magmas, based on the partial melting of the continental crust, caused by the rise of mafic magma.