The galaxy presents as a relatively smooth, centrally concentrated object. Its overall shape appears to be elliptical, with the isophotes appearing mostly round but trending towards being in between round and elongated. There is no obvious disk structure or spiral arms visible. The central region is significantly brighter than the outer regions, suggesting a higher density of stars or active galactic nucleus activity. There are no obvious signs of recent mergers or major tidal disturbances, although minor irregularities are difficult to resolve at this resolution. The color appears relatively uniform across the galaxy.