The galaxy presents as a relatively smooth, lenticular structure. It is elliptical in shape, with a bright, concentrated central bulge that dominates the overall luminosity. The halo appears to gradually fade, indicating a lack of distinct, well-defined spiral arms or significant dust lanes. The color gradient suggests an older stellar population, with the core appearing more yellow and the outer regions a bit more red. There is a possible minor asymmetry or disturbance in the outer halo on the right side. This could indicate a past interaction or merger event, however, it is mostly smooth and undisturbed. Overall, the galaxy appears to be a relatively evolved, quiescent system.
