The galaxy presents as a moderately luminous, relatively compact system. It appears predominantly smooth in texture with minimal discernible substructure. The overall shape is broadly elliptical, with a high degree of circularity. There is a suggestion of a slight extension or plume-like feature emanating from the lower edge of the galaxy. This could indicate tidal interactions or some form of disturbance. The color appears to be primarily in the redder part of the spectrum, possibly indicating an older stellar population and lower levels of current star formation. The central region of the galaxy seems to be brighter than the surrounding areas. There is no apparent disk component or spiral arm structure evident in this imagery. No other galaxy mergers are seen.
