The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits an elliptical morphology, appearing nearly circular in projection. The light profile suggests minimal substructure, with a gradual decline in brightness from the core to the outer regions. There is a subtle color gradient, with the central region appearing slightly yellower and the outskirts exhibiting a bluer tint, suggestive of ongoing or recent star formation. No prominent tidal features or signs of major mergers are discernible. Minor disturbances may be present in the disk.
