The galaxy presents as a relatively smooth, centrally concentrated object. It appears to have an elliptical morphology. The core is characterized by a yellowish-white hue, which may indicate an older stellar population. Moving outward from the core, the light gradually fades. There is a slight indication of bluer colors in the outer regions, hinting at the possibility of some ongoing star formation, though the overall color suggests a galaxy dominated by older stars. No strong spiral arm structures or significant dust lanes are apparent, and there is no evidence of any major tidal disturbances or mergers.
