The galaxy presents as a largely featureless elliptical or lenticular galaxy. Its overall shape is consistently round, indicating minimal rotational support. The light distribution is smooth and centrally concentrated, with a gradual decrease in intensity outwards from the core. There is no apparent spiral arm structure, nor any distinct disk component visible. Color gradients are subtle, with a slight shift toward redder hues in the central region. The absence of prominent dust lanes or star-forming regions suggests a relatively quiescent galaxy, possibly in the process of, or having completed, its transition toward a passively evolving system. There are no indications of significant interactions or merging events.
