The galaxy appears to be a relatively smooth, centrally concentrated object. It exhibits a largely elliptical morphology with a high degree of roundness. There is no obvious presence of spiral arms, bars, or significant disk structures; it seems to be more akin to a spheroid. There is a slight colour gradient, with a somewhat bluer hue present in the outskirts of the galaxy, transitioning toward a redder colour closer to the center of the galaxy. There is no obvious indication of a major merger event and the overall structure appears relatively undisturbed. The light profile appears generally uniform and well-defined, indicating the galaxy is in a relatively stable state.
