The galaxy presents as a somewhat diffuse, luminous object. Its morphology appears predominantly smooth, with a concentrated central bulge exhibiting a yellowish hue. Fainter, bluer light extends outwards from the bulge in a more disc-like structure. There may be subtle asymmetries or minor disturbances in the outer regions of the disk. These features are consistent with the possibility of some recent star formation. The color suggests a system dominated by older stellar populations, particularly towards the core, although some younger stars may be present in the outer regions. The relative lack of discernible spiral structure or prominent dust lanes suggests that if this galaxy is a spiral, it is of the later type, possibly a lenticular galaxy.
