The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge that is bright and yellowish in color, suggesting a population of older stars. There is little evidence of spiral arm structure or significant dust lanes. The light gradually fades toward the outer edges, indicating a diminishing stellar density further from the galactic center. Overall, the galaxy appears to be a relatively undisturbed system, without any signs of major tidal interactions or mergers.
