The galaxy presents as a generally smooth, elliptical object. The light is concentrated toward the center of the galaxy, with a noticeable decrease in luminosity towards the outer regions. The color profile indicates a redder central bulge transitioning to a slightly bluer halo, suggestive of an older stellar population centrally with the possibility of some younger stars in the outskirts. There are no distinct spiral arms or features indicating recent or ongoing major mergers. Overall, it appears to be a well-defined, relatively undisturbed galaxy.
