The galaxy presents as a relatively smooth, centrally concentrated object with a generally elliptical morphology. There is a pronounced central bulge, which appears to be the brightest region, suggesting a high stellar density. The overall color profile indicates a population of older stars. There is no evidence of spiral arms or significant dust lanes. It exhibits minimal signs of recent or ongoing star formation. There are no apparent signs of tidal disturbances or ongoing mergers. The outer regions of the galaxy appear somewhat diffuse, gradually fading into the background sky.
