The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a centrally concentrated bulge, characterized by a luminous, nearly uniform light distribution with a slightly redder hue than its surrounding area. Fainter, bluer light extends outwards, forming a disk-like component. The shape deviates from a perfect circle, appearing more elongated. There appears to be a very minor degree of disturbance, but its overall shape is mostly undisturbed. The galaxy displays a relatively low rate of star formation.
