The galaxy presents as a centrally concentrated object, appearing largely smooth in texture with minimal discernible substructure. Its overall morphology suggests an elliptical galaxy. The core region exhibits a higher luminosity, indicating a denser concentration of stars. The light profile appears to gradually fade from the center outwards, without evidence of spiral arms or a prominent disk component. There may be a slight bluing in the central part of the galaxy indicating more recent star formation there. No strong signs of tidal disturbances or ongoing mergers are apparent in this image. The overall color index suggests a mature stellar population. The galaxy seems to be in a relatively quiescent state, with a small but existent amount of star formation. It is neither perfectly circular nor highly elongated.
