The galaxy presents as a relatively smooth, elliptical structure with a concentrated central bulge. There appears to be a lack of distinct spiral arm features. Color gradients suggest a redder core region, possibly indicative of an older stellar population, while the outer regions seem slightly bluer, implying the presence of some younger stars or ongoing, albeit limited, star formation. The galaxy's overall shape exhibits a minor ellipticity, appearing almost circular. There is no clear visual evidence of any major ongoing merger activity or significant tidal disturbances. Overall, the galaxy seems to be an evolved, relatively undisturbed system.
