The galaxy presents as a lenticular or edge-on spiral morphology. It exhibits a smooth, elongated central bulge that dominates the overall structure. There is evidence of a flattened disk component viewed nearly edge-on. The disk appears relatively thin and lacks prominent spiral arm structures, although there is a faint blue tinge along some regions of the disk, which may indicate recent star formation activity. Dust lanes are either absent or not easily discernible within the limitations of the image resolution. The galaxy appears to have a relatively low surface brightness, with a gradual falloff in luminosity from the central region outwards. Its overall light profile suggests that it is likely an early-type spiral or lenticular galaxy with a low star formation rate.
