The galaxy presents a generally smooth and rounded morphology. There is a bright central region that dominates the galaxy's light output, suggesting a concentration of older stars and potentially a supermassive black hole actively accreting material. A very faint extended halo or disk-like structure can be observed around the bright central region, however it is mostly featureless, showing little to no spiral arm structure. The colors suggest that we are dealing with a galaxy with primarily older stellar populations. The absence of significant dust lanes or prominent star-forming regions supports this interpretation. Overall, this galaxy appears to be a relatively evolved system with a well-defined elliptical or lenticular shape. There does not appear to be any merger activity occurring, nor any tidal features.
