This galaxy appears to be an elliptical galaxy at a considerable distance, evidenced by its relatively small angular size. The light distribution exhibits a smooth profile with a central concentration, gradually decreasing in intensity outwards. The galaxy's shape is generally round, with minimal deviation from circular symmetry. The color profile suggests a population of older stars, with a bias towards redder wavelengths in the central region. There is no distinct disk structure, spiral arms, or prominent dust lanes visible. There is little indication of ongoing major star formation. The galaxy seems relatively undisturbed with no clear signs of recent or ongoing mergers or tidal interactions. There is a very faint bluish hue around the edges of the galaxy, possibly indicating a small amount of recent star formation on the outskirts.
