The galaxy presents as a centrally concentrated object, appearing largely smooth in morphology. There is a gradual fading of luminosity from the center outwards, showing a lack of distinct features such as spiral arms or a prominent bar. The light profile suggests an elliptical or lenticular classification, with the overall shape appearing close to circular. Its color index suggests the presence of an older stellar population dominating the galaxy's light output. Star formation seems to be relatively quiescent. There's no visible evidence of tidal disturbances or ongoing mergers. The apparent size is relatively compact indicating that this is a massive galaxy at cosmological distance.
