The galaxy presents as an elliptical morphology, with a high degree of smoothness. Its light profile indicates a concentrated central bulge that gradually fades into the outer regions of the galaxy. There is a noticeable elongation of the galaxy along one axis, resulting in an oval appearance. The colour appears to be redder toward the galactic nucleus and becomes slightly bluer in the outer regions. There is no indication of spiral arms or significant dust lanes. No active star formation regions are obviously visible.