The galaxy presents a primarily smooth, elliptical morphology. There is a bright central bulge that appears roughly circular. The luminosity is fairly high, indicating a potentially high stellar mass. The galaxy appears to be a relatively isolated system, showing no signs of major mergers or significant tidal disturbances, however, there is a small secondary galaxy nearby. Overall, the galaxy exhibits a high degree of symmetry and smoothness, indicative of an evolved system, but may have minor star formation.
