The galaxy presents a largely smooth morphology, suggestive of an elliptical or lenticular type. The light distribution is centrally concentrated with a gradual decrease in intensity outwards. There is a slight elongation. The central region exhibits a yellowish hue, possibly indicating an older stellar population. The outer regions show a hint of bluer colors, potentially associated with pockets of younger stars, although these features are not highly pronounced. No obvious spiral arms or dust lanes are visible. There is no strong evidence of a recent major merger event, though subtle distortions might suggest minor interactions.
