The galaxy presents a largely smooth and elliptical morphology. Its light profile is concentrated towards the center, indicating a substantial bulge component. The central region exhibits a yellowish-white hue, suggestive of an older stellar population. The outer regions fade into a bluish tint, potentially indicative of some ongoing, albeit low, star formation activity. There's a possible minor disturbance in the form of a slight asymmetry in its overall shape, though no clear signs of ongoing major mergers are observed. It appears to be relatively isolated, with no nearby companions visibly interacting.
