The galaxy presents as a largely smooth, elliptical-like structure with a concentrated central bulge. The light distribution appears centrally peaked, with a gradual decrease in intensity moving outward from the core. There is a clear color gradient, transitioning from a yellowish core to a redder halo or outer region, suggesting a population shift from relatively younger to older stars, respectively. The overall morphology suggests a system that is not currently undergoing a major merger event. There is a very slight indication of a possible minor disturbance, such as a faint tidal feature, on one side of the galaxy, though it is very subtle.
