This galaxy appears to be a relatively smooth, elliptical galaxy, exhibiting a bright, concentrated central bulge that fades into a more diffuse halo. The galaxy is generally elliptical in shape, appearing mostly rounded but somewhat in between round and cigar shaped, with minimal indication of spiral arms or a distinct disk structure. There are no obvious signs of ongoing mergers or major disturbances within its structure, though subtle irregularities in the outer regions cannot be ruled out. The color profile suggests a population of older stars, with a somewhat subdued presence of younger, blue stars, implying a relatively low star formation rate. Overall, the galaxy presents as a relatively quiescent system, likely past its peak of star formation activity.
