The galaxy presents as a relatively smooth, elliptical object. The light distribution appears concentrated towards the center, suggesting a prominent galactic nucleus or bulge. There may be a faint disk-like structure surrounding the central bulge, but that is not certain. The galaxy does not exhibit any strong tidal features or other signs of major mergers or interactions with other galaxies. The color profile indicates that the galaxy is likely a more evolved system with a population of older stars, emitting less light in the blue end of the spectrum. The overall structure seems undisturbed, showing no significant distortions or asymmetries.
