This galaxy appears to be a relatively smooth, elliptical-like system. It exhibits a concentrated central bulge, with a gradual decrease in luminosity extending outwards. The color profile suggests a dominant population of older stars, imparting a yellowish-red hue. There is no clear evidence of spiral arm structures or significant dust lanes, and the overall morphology indicates a relaxed system without obvious signs of recent major mergers or tidal disturbances. A possible minor disturbance is suggested on the north-east side of the galaxy, though it could simply be a foreground object.
