The galaxy presents as a dominant, centrally located, relatively smooth elliptical system. It exhibits a bright, concentrated core, surrounded by a more diffuse halo that gradually fades into the background sky. The color appears to be predominantly yellowish-orange, suggesting an older stellar population with relatively little ongoing star formation. There is no apparent spiral arm structure or significant dust lanes visible in this image. The overall morphology suggests a relaxed system, perhaps a product of previous mergers, with a high degree of symmetry. No strong tidal features or signs of recent interactions are immediately apparent, though subtle disturbances might be present upon closer inspection.
