The galaxy presents as a relatively smooth, elliptical-like structure. Its core region exhibits a bright, concentrated luminosity, while its outer regions gradually decrease in intensity. There is a subtle suggestion of a disk, yet it is very faint. The overall color profile leans toward a redder hue. There are no obvious signs of ongoing major mergers or significant tidal disturbances and no strong evidence of intense star formation. The galaxy displays a fairly regular, rounded shape with minimal deviations. It may have experienced minor gravitational interactions in its past, but this is only slightly evident. The estimated physical size is a few kiloparsecs.
