The galaxy presents as an elliptical morphology. It exhibits a smooth, centrally concentrated light distribution, lacking prominent spiral arms or a distinct disk structure. The central region displays a bright, relatively compact core, potentially indicative of a supermassive black hole or a dense concentration of stars. The overall color profile suggests a population dominated by older, redder stars. The galaxy appears relatively undisturbed with no significant signs of on-going major mergers or tidal interactions. There is a suggestion of a minor structural asymmetry within the central region but it is not definitive.
