The galaxy appears as an elliptical or lenticular type. It presents a relatively smooth, centrally concentrated light profile, with a bright core that diminishes outwards. The overall color is slightly redder, potentially indicating an older stellar population or the presence of dust. There may be a hint of a faint disk-like structure or slight flattening, but this is not highly pronounced. There are potentially some disturbances in the shape. It shows no distinct spiral arms, and appears relatively undisturbed, with no indications of major ongoing mergers, though a minor disturbance cannot be ruled out. It does not appear particularly round.
