The galaxy presents a generally smooth, elliptical morphology. Its core exhibits a bright, concentrated luminosity, suggestive of a high stellar density and potentially the presence of a supermassive black hole. Proceeding outwards, the galaxy gradually fades into a less luminous halo. The galaxy appears relatively undisturbed with no significant signs of mergers or tidal interactions. The color profile of the galaxy shows a subtle red shift, which may be due to distance. It also suggests an aging stellar population throughout the galaxy. There are no evident spiral arms or dust lanes.
