The galaxy appears to be a relatively smooth, elliptical system. It exhibits a concentrated, bright central bulge, possibly indicating an older stellar population. The overall shape is somewhat elongated, with a slight flattening. A faint, diffuse halo surrounds the central region, gradually fading into the background. Subtle color variations suggest some level of ongoing or recent star formation, although the dominant stellar population appears to be older. There is a hint of disturbance in the outer regions, suggestive of a possible past interaction or merger event, though this is not immediately apparent.
