The galaxy presents as a moderately luminous, relatively compact system. Its morphology appears largely spheroidal, suggesting it might be an elliptical galaxy or a lenticular galaxy viewed face-on. The central region exhibits a brighter, concentrated luminosity profile, possibly indicative of an older stellar population or a weak active galactic nucleus. The outer regions fade gradually, without clear spiral arm structures or significant dust lanes visible. Overall, the galaxy exhibits a smooth, featureless appearance, which implies a quiescent star formation history. There may be weak signs of past merging or tidal interactions.
