The galaxy presents as a somewhat amorphous, centrally concentrated object. Its overall color suggests a mix of stellar populations. The inner region is dominated by light with yellower hues, possibly indicating an older stellar population. Moving outwards, the galaxy exhibits a more diffuse profile with hints of bluer regions. Patches of light indicate areas of enhanced activity. These regions could be due to either recent star formation or tidal disruptions due to galaxy mergers. There is some indication of minor disturbances.
