The galaxy appears to be a relatively smooth, elliptical system. It exhibits a concentrated central bulge that fades into a more diffuse halo. The overall color profile suggests a population of older stars, with a general lack of prominent blue star-forming regions. The morphology indicates a relaxed structure, with no significant tidal features or signs of recent major mergers. Minor irregularities in the outer regions may point to past interactions or minor disturbances. It exhibits a moderate degree of roundness, not appearing particularly flattened or elongated. It seems to be a fairly massive galaxy, though with a relatively low rate of star formation.
