The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge, with a gradual decrease in luminosity extending outwards. There is little indication of spiral arm structures or prominent dust lanes. The overall color is subtly reddish, suggesting an older stellar population and relatively low ongoing star formation activity. The galaxy appears relatively isolated and does not seem to be undergoing any major merging events or significant tidal disturbances, although there is a possible minor disturbance present. The galaxy has a high smoothness fraction and is round-shaped.
