The galaxy presents as a relatively smooth, centrally concentrated object. The core region exhibits a bright, yellowish-white luminosity, suggesting an older stellar population dominating the central bulge. Moving outwards from the core, there is a gradual decrease in surface brightness. The overall shape appears largely elliptical, deviating only slightly from a perfect circle. There is a faint disk of bluer color, suggesting regions of active star formation. There are no obvious signs of spiral arm structures or major disturbances indicative of recent or ongoing mergers. The galaxy displays a notable level of symmetry, with no clear asymmetries in its light distribution. Overall, the galaxy appears to be a well-formed system, likely on the red sequence.
