The galaxy presents a generally smooth, elliptical morphology, with a high degree of circularity. There is a bright, concentrated central bulge which appears yellow-white in color, indicating an older stellar population. This region is surrounded by a more diffuse halo extending outwards, fading into the background. The halo exhibits a slightly bluer hue compared to the bulge, which could suggest the presence of a younger stellar population and ongoing star formation, albeit at a relatively low rate. No distinct spiral arms or bars are visible. The galaxy appears to be relatively undisturbed, showing no clear signs of recent major mergers or tidal interactions. Its overall structure is consistent with an early-type galaxy at intermediate redshift.
