The galaxy presents as a centrally concentrated, relatively smooth object. Its morphology appears primarily elliptical, with a high degree of roundness. There is a noticeable color gradient, with a central, yellowish core region transitioning to a bluer halo. The halo appears diffuse, lacking significant distinct features. No pronounced spiral arms, bars, or dust lanes are evident in the image. The overall structure suggests a evolved system, potentially undergoing ongoing star formation but at a rate that does not dominate its appearance. The lack of major disturbances implies the galaxy has likely not undergone a recent major merger event, although minor interactions cannot be entirely ruled out. The galaxy is moderately luminous, indicating it is a fairly massive system.
