The galaxy presents a primarily smooth morphology, exhibiting a softly rounded shape. The central region appears to be considerably brighter than the outer regions, suggesting a concentration of older stars or a possible active galactic nucleus. While mostly smooth, there are hints of subtle structural features possibly indicating a weak disk-like component or some past minor disturbances. The color profile indicates a significant population of older stars, but possibly with some ongoing star formation. There is no strong evidence of any major ongoing mergers or interactions. The galaxy is likely a relatively massive system.