The galaxy presents as a moderately bright, somewhat elliptical structure. It displays a smooth, diffuse morphology without prominent spiral arms or a well-defined bar. The core region appears significantly brighter and exhibits a yellowish or slightly orange hue, suggesting an older stellar population. The outer regions of the galaxy fade into a more diffuse halo, showing hints of a bluer tint, potentially indicating the presence of younger stars or ongoing star formation, albeit at a low rate. There is a subtle suggestion of a disk-like component, though the overall structure appears dominated by a spheroid. No signs of major mergers or significant tidal disturbances are readily apparent in the image, however, there is slight asymmetry and a small amount of disturbance on the left side of the galaxy.
