The galaxy presents a largely smooth, elliptical morphology. The light distribution is highly concentrated towards the center, indicating a prominent galactic nucleus. A smooth halo extends outwards, with colors gradually shifting to a redder hue. The overall roundness is close to circular, with no obvious signs of strong tidal disturbances or major mergers. Subtle features suggest that there might be ongoing minor interactions or internal processes influencing its structure. The galaxy is relatively bright, appearing as a well-defined object in the image.
