The galaxy presents a generally smooth and elliptical morphology. The light distribution is centrally concentrated, with a bright core that gradually fades into the outer regions. There appears to be a lack of distinct spiral arm structures or prominent dust lanes. The galaxy exhibits a subtle color gradient, appearing slightly bluer towards the periphery, possibly indicating the presence of a younger stellar population in the outer regions, while the central bulge seems more yellow/red. The overall roundness suggests a classification toward the earlier end of the Hubble sequence. No signs of major mergers or significant tidal disturbances are apparent in the image.
