The galaxy appears to be a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge that fades outward into a more diffuse halo. The overall shape approximates a rounded form, though a slight elongation is noticeable. There's minimal indication of spiral arms or significant dust lanes. The color profile suggests a primarily older stellar population with a yellowish-white hue in the central regions, transitioning to slightly bluer tones in the outer regions, potentially indicating some ongoing, albeit subdued, star formation. There are no indications of any major mergers or strong tidal distortions. It appears to be a fairly isolated system undergoing relatively quiescent evolution.
