The galaxy appears to be a relatively smooth, elliptical system. It exhibits a concentrated central bulge, characterized by a yellow-white hue. The outer regions show a gradual decrease in surface brightness, with a subtle transition to a slightly bluer color. There is no discernible spiral arm structure. The overall morphology suggests an evolved stellar population, with little evidence of recent major merger activity or significant star formation. The galaxy appears generally round in shape, with only minor deviations from perfect circularity.
