In the present work, we study the noncommutative version of a quantum cosmology model. The model has a Friedmann–Robertson–Walker (FRW) geometry, the matter content is a radiative perfect fluid and the spatial sections have zero constant curvature. In this model, the scale factor takes values in a bounded domain. Therefore, its quantum mechanical version has a discrete energy spectrum. We compute the discrete energy spectrum and the corresponding eigenfunctions. The energies depend on a noncommutative parameter [Formula: see text]. We compute the scale factor expected value ([Formula: see text]) for several values of [Formula: see text]. For all of them, [Formula: see text] oscillates between maxima and minima values and never vanishes. It gives an initial indication that those models are free from singularities, at the quantum level. We improve this result by showing that if we subtract a quantity proportional to the standard deviation of [Formula: see text] from [Formula: see text], this quantity is still positive. The [Formula: see text] behavior, for the present model, is a drastic modification of the [Formula: see text] behavior in the corresponding commutative version of the present model. There, [Formula: see text] grows without limits with the time variable. Therefore, if the present model may represent the early stages of the universe, the results of the present paper give an indication that [Formula: see text] may have been, initially, bounded due to noncommutativity. We also compute the Bohmian trajectories for [Formula: see text], which are in accordance with [Formula: see text], and the quantum potential [Formula: see text]. From [Formula: see text], we may understand why that model is free from singularities, at the quantum level.