The galaxy presents as a generally smooth, elliptical-like structure. It exhibits a concentrated central bulge with a diffuse halo extending outwards. The color profile suggests a higher concentration of older stellar populations within the core region, indicated by the yellowish-orange hue. The outer regions appear slightly bluer, potentially indicating the presence of younger stars, although this is less pronounced. There are no obvious signs of spiral arms or significant dust lanes. The overall morphology is relatively undisturbed, without any prominent tidal features or indications of recent major mergers. A slight elongation is visible, departing somewhat from a perfectly circular shape. The structure is consistent with an early-type galaxy that is not currently undergoing intense star formation.
