The galaxy presents an elliptical morphology. The light distribution appears relatively smooth, with a high degree of central concentration. The overall color is yellowish-orange, suggesting a population of older stars and a low rate of ongoing star formation. There is no indication of spiral arms or a prominent disk. The galaxy is moderately elongated, appearing more "in-between" than perfectly round or cigar-shaped. There is no obvious evidence of major mergers or significant tidal disturbances, though minor distortions are plausible. 
