The galaxy presents a primarily smooth morphology, appearing as an elliptical or lenticular type. It displays a generally rounded shape, though not perfectly circular. There are no clear signs of major disturbances, such as tidal tails or strong asymmetries suggesting an ongoing or recent major merger event. Faint color gradients suggest the presence of differing stellar populations within the galaxy. The galaxy appears relatively quiescent in terms of star formation activity, as evidenced by the lack of prominent blue regions associated with young, hot stars. Faint irregular features suggest very minor disturbances or internal processes.
