The galaxy appears to be elliptical in shape, exhibiting a smooth morphology with no discernible spiral arms or a distinct disk. It presents a concentrated, bright central bulge that transitions gradually into a fainter, more diffuse halo. The galaxy appears largely undisturbed, showing no obvious signs of ongoing mergers or major tidal disruptions. The color profile suggests a population of older stars, indicated by the reddish-yellow hue, particularly prominent in the central regions. There may be some indications of ongoing star formation, as suggested by some bluer regions in the outer parts of the galaxy, though not very distinct. The overall structure and light distribution imply a relatively evolved system with a significant stellar mass.
