The galaxy presents a relatively smooth and rounded appearance. It is elongated in shape, appearing somewhat cigar-shaped. The galaxy exhibits a concentration of light towards its center, indicating a bulge component. There is some evidence of a disturbance in the morphology, which may indicate a minor merger, but the central region of the galaxy is relatively undisturbed. The color profile suggests a population of older stars within the primary body of the galaxy. Star formation rates are estimated to be very low. Overall, the galaxy appears to be a relatively massive system, likely an early-type galaxy with a red color and passive star formation.
