The galaxy presents as a relatively smooth, elliptical or lenticular structure. Its central bulge is prominent and appears reddish in color, possibly indicative of an older stellar population. There is a subtle disk-like structure surrounding the bulge with hints of bluer colors, which could suggest ongoing, albeit low-level, star formation. The galaxy lacks a distinct spiral arm structure or prominent dust lanes. Its overall shape appears to be somewhere between round and elongated. There are no obvious signs of major mergers or tidal disturbances, although there could be a minor interaction with another galaxy due to some slight asymmetry in its outer regions. The galaxy has an apparent size which is consistent with a moderate luminosity.
