The galaxy presents as a moderately luminous, elliptical-shaped structure. Its light profile appears relatively smooth and centrally concentrated, with a bright, yellowish core indicative of an older stellar population likely dominating the nuclear region. Moving outward from the core, the galaxy gradually fades into a diffuse halo, displaying a subtle color gradient with slightly bluer hues. The overall morphology suggests a system that is primarily supported by random stellar motions. There is a minor disturbance in the symmetry of the disk. Based on the apparent size and characteristics, it is possible the galaxy has experienced past or ongoing interactions. The observed color and morphology together tentatively suggest a system with a relatively low ongoing star formation rate.
