The galaxy presents as a roughly elliptical structure, demonstrating a smooth overall appearance. There is a brighter central bulge that fades into the outer regions of the galaxy. No distinct spiral arms or bar structures are clearly visible. The galaxy appears to be relatively undisturbed, lacking any significant signs of ongoing merging activity or major tidal disruptions, although minor disturbances cannot be ruled out. Color gradients suggest a stellar population that is slightly redder in the central regions, potentially indicating older stars, with bluer colors becoming more prevalent in the outskirts, possibly hinting at younger stars in the outer regions. The overall morphology is consistent with an early-type galaxy, possibly an elliptical or lenticular type.
