The galaxy presents as a centrally concentrated, smooth object with a generally elliptical morphology. The light distribution exhibits a radial gradient, with a bright, compact core region transitioning to a fainter, more diffuse halo. There is a slight elongation, deviating somewhat from a perfect circular shape. The color profile suggests a population of older stars, as indicated by the redder hues of the central bulge. There is no strong evidence of spiral arm structures or prominent dust lanes; however, there might be some faint disk-like features. There may be some minor star formation in the extended regions, and there are no signs of major ongoing mergers or significant tidal disturbances.
