The galaxy presents a generally elliptical morphology, appearing quite smooth and concentrated towards the center. The core region exhibits a yellowish-white hue, potentially indicative of an older stellar population. The isophotes appear fairly regular and concentric, suggesting a relaxed system.

There is a subtle color gradient extending outwards from the core. The outer regions display a slightly bluer tint compared to the central bulge, which may indicate the presence of some younger stars or ongoing, albeit subdued, star formation in the outer disk. There is also a hint of a tidal feature or minor disturbance located on one edge, suggestive of a past interaction or accretion event. This feature seems to be separate from the main body of the galaxy. It is otherwise largely undisturbed in appearance.
