The galaxy presents a generally smooth, elliptical morphology. Its light profile appears centrally concentrated, with a gradual decrease in surface brightness outwards from the core. The primary color is a yellowish-orange, indicative of a stellar population dominated by older, redder stars. Faint bluish features are observed in the galaxy's outer regions, potentially suggesting regions of more recent, albeit limited, star formation. There appears to be no clear spiral arm structure or significant dust lanes, which is consistent with its classification as a smooth, elliptical galaxy. Faint disturbances may exist. There is no evidence of ongoing major merger activity.
