The galaxy appears to be an elliptical type, characterized by its smooth, relatively featureless structure. It exhibits a high degree of central concentration, with a bright core that gradually fades into the surrounding halo. The overall shape is roughly circular, though not perfectly so. There is some suggestion of minor asymmetry or disturbances, possibly indicative of a past interaction or merger event. The color profile suggests a relatively older stellar population, with a redder hue dominating the outer regions, transitioning to a somewhat bluer tint toward the center. There is no discernible spiral arm structure or significant dust lanes. The low level of recent star formation agrees with the redder color profile.
