Studies of Galactic H ii regions are of crucial importance for studying star formation and the evolution of the interstellar medium. Gaining an insight into their physical characteristics contributes to a more comprehensive understanding of these phenomena. The GLOSTAR project aims to provide a GLObal view on STAR formation in the Milky Way by performing an unbiased and sensitive survey. This is achieved by using the extremely wideband (4$-$8 GHz) C -band receiver of the Karl G. Jansky Very Large Array and the Effelsberg 100 m telescope. Using radio recombination lines observed in the GLOSTAR survey with the VLA in D-configuration with a typical line sensitivity of 1\,$ 3.0 mJy $ at $ 5 km $ and an angular resolution of 25 we cataloged 244 individual Galactic H ii regions ($-$2$ ell leq 60degr b | leq 1degr and 76$ ell leq 83degr b leq 2degr ) and derived their physical properties. We examined the mid-infrared (MIR) morphology of these H ii regions and find that a significant portion of them exhibit a bubble-like morphology in the GLIMPSE 8 mu m emission. We also searched for associations with the dust continuum and sources of methanol maser emission, other tracers of young stellar objects, and find that 48<!PCT!> and 14<!PCT!> of our H ii regions, respectively, are coextensive with those. We measured the electron temperature for a large sample of H II regions within Galactocentric distances spanning from 1.6 to 13.1 kpc and derived the Galactic electron temperature gradient as sim 372 pm 28 K kpc$^ $ with an intercept of 4248 pm 161 K, which is consistent with previous studies.