This galaxy appears to be a relatively smooth, elliptical-like system. It presents a concentrated central bulge that is bright and appears yellowish-orange. The outer regions display a gradual decrease in luminosity moving outwards from the center. There is some asymmetry, suggestive of a slight tidal disturbance or past merger event with the disk of the galaxy extending slightly more towards the bottom left. The overall color profile suggests a population of older stars, with less ongoing star formation.
