The galaxy presents an overall elliptical morphology, appearing somewhat compact. Its central region is characterized by a noticeable brightness concentration, indicating the presence of a nucleus or a dense central bulge. The light distribution appears relatively smooth, with no obvious spiral arm structures or significant dust lanes visible. There is a slight asymmetry observed in the outer regions of the galaxy, potentially indicative of a minor tidal interaction or disturbance. Color variations across the galaxy are subtle, with a suggestion of a redder hue, concentrated in the central region which could be from older star populations, while outer regions exhibit a slightly bluer tone. The galaxy appears relatively isolated, without any nearby companions immediately apparent in the frame, though subtle distortions suggest it has a history with tidal disturbances.
