The galaxy presents as a smooth, centrally concentrated elliptical morphology. It exhibits a high degree of circular symmetry, with minimal apparent distortion or tidal features suggesting recent major merger activity. A bright, well-defined core region transitions gradually into a diffuse halo.

There is some color variation within the galaxy. The central region appears more yellow-white, suggestive of an older stellar population. The outer halo displays a bluer hue, potentially indicative of ongoing, albeit modest, star formation activity or a population of younger stars.
