The galaxy presents a largely smooth, elliptical morphology. Its light profile exhibits a high degree of central concentration, suggesting an older stellar population dominates its core. There is a subtle color gradient, with the central regions appearing somewhat bluer than the outer halo. The overall red color suggests that the galaxy is composed largely of older stars and has not been actively forming stars for some time. Although it appears mostly smooth, there is some slight evidence of features, perhaps a minor disturbance, which might indicate that the galaxy is currently undergoing or has undergone a minor merger in the past. No prominent spiral arms or dust lanes are visible. The overall shape appears mostly round.