The galaxy presents as a somewhat compact, relatively smooth, and centrally concentrated object. The light distribution appears mostly elliptical with a high degree of roundness, showing no obvious signs of a disk component or spiral structure. There is a gradual decrease in brightness from the center outwards, but the image resolution does not allow for a clear identification of any distinct internal structures such as a bar or rings. The overall color appears to be slightly reddish, suggesting a population of older stars. There is no obvious evidence of strong tidal interactions, major mergers, or significant star formation regions based on visual inspection of the image.
