The galaxy presents a primarily smooth morphology, suggestive of an elliptical or lenticular type. There is some indication of a disk or perhaps faint spiral arms in the outer regions, but these features are not sharply defined. The central bulge exhibits a higher surface brightness and a yellowish color, possibly indicating an older stellar population. The outer regions of the galaxy appear bluer, which is indicative of ongoing or recent star formation activity. The shape is relatively round. There is no clear evidence of major tidal disturbances or an ongoing merger, although some minor asymmetry might be present. Overall, the galaxy appears to be a mature system with a combination of both old and younger stellar populations and low levels of star formation.
