The galaxy presents as a relatively smooth, elliptical-shaped object. It exhibits a bright, concentrated core region which appears to have some activity in its center. Moving outward from the core, a more diffuse, halo-like structure is observed. The color gradient suggests a stellar population that is relatively evolved, with some ongoing, but slow, star formation. There is a hint of faint, extended features, potentially indicating tidal interactions or minor disturbances. The overall appearance is consistent with a galaxy that is not actively undergoing a major merger event.
