The galaxy presents as an elliptical morphology, with a smooth, centrally concentrated light profile. There is a bright core, indicating a likely high stellar density. The color index, estimated from the red and blue light emissions, suggests a population dominated by older, redder stars. The overall shape is roughly round, but exhibits a slight elongation. Faint disturbed features are present along its outskirts, these could potentially be tidal streams or other minor interactions. The presence of these disturbances warrants further investigation, as they may indicate past or ongoing merging events. There is some potential dust obscuration, however, overall it presents as a mature system with little active star formation.
