The galaxy appears to be a lenticular or early-type spiral galaxy, characterized by a prominent bulge and a relatively faint disk. The central bulge exhibits a smooth, concentrated light profile, suggesting an older stellar population. The disk appears to be viewed at a moderate inclination, and it displays a subtle blue tint, indicative of some ongoing star formation. There is a slight asymmetry in the light distribution of the disk with a hint of a possible tidal interaction, or a merging event in the past. It is neither strongly disturbed nor undergoing a major merger. There are no apparent dust lanes or spiral arm structures, which, coupled with the dominant bulge, is consistent with the appearance of a galaxy that may have exhausted most of its gas supply, and has a low star formation rate. The overall morphology suggests an intermediate stage in the morphological transformation of galaxies.
