The galaxy presents as a largely featureless, smooth elliptical system. It exhibits a concentrated, bright central bulge which graduates outward into a more diffuse halo. The color profile indicates a higher concentration of older stellar populations, particularly in the central regions, appearing more yellow-reddish. There is no discernible spiral structure or active star forming regions visible in the image; the morphology suggests a quiescent system. The generally round shape suggests it is likely not undergoing major merger activity.
