This galaxy presents as a relatively compact and smooth system. Its morphology appears to be elliptical, exhibiting a high degree of circular symmetry in its overall form, with very little distortion. There is a minor variation in color across the galaxy, with slightly bluer hues appearing near the center. This may indicate regions of slightly younger stellar populations or on-going star formation. However, the overall color suggests that the galaxy is composed primarily of older stars. There are no prominent dust lanes or spiral arm structures visible. There is no visually apparent indication of major disturbances due to mergers or tidal interactions with other galaxies, as the galaxy appears undisturbed.
