The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge that gradually fades outwards into a more diffuse halo. The color profile appears mostly homogenous, with a yellow-red hue, which suggests a population of older stars. There is no obvious sign of active star formation within the galaxy itself. The morphology is generally undisturbed, showing no prominent tidal features or indications of recent major mergers. The roundness of the galaxy is high, with the galaxy being nearly circular.