The galaxy exhibits a smooth, elliptical morphology, displaying a generally round shape, though with some slight elongation. The central bulge is prominent and appears uniformly bright, yellow in color indicating an older stellar population. No distinct spiral arm structure or dust lanes are discernible. A faint, diffuse halo surrounds the central region, gradually fading into the background sky. There are no signs of any major interactions or tidal disturbances, and it appears relatively undisturbed. The color gradient suggests a higher concentration of older stars in the core, with a bluer, potentially younger stellar population in the outer regions, though this is subtle.