The galaxy presents as a centrally concentrated, largely featureless, elliptical-like structure. The light profile appears smooth and generally round, showing a high degree of symmetry. The color index suggests a higher concentration of older stellar populations. The lack of apparent spiral arms, dust lanes, or significant tidal features indicates a relatively quiescent state, devoid of ongoing major merging activity. The small size and high degree of smoothness indicate that it is likely a massive galaxy that is no longer forming stars. There may be weak presence of a disk.
