The galaxy presents as a relatively smooth, elliptical structure with a bright, concentrated central bulge. There is a faint suggestion of a disk, evidenced by a slight flattening and extension along one axis, however, distinct spiral arms are absent. The overall color is consistent with an older stellar population, trending towards redder hues. Based on the smoothness and light profile, the galaxy can be classified as an early-type galaxy. The lack of significant morphological disturbances suggests that it is relatively undisturbed and not currently undergoing a major merger event. 
