The galaxy presents as two primary components. Each component displays a roughly circular morphology with a smooth, concentrated light profile, suggestive of an elliptical or spheroidal structure. The color appears predominantly reddish-orange, possibly indicating an older stellar population and/or significant dust extinction. There is a faint bluish-green halo of light that surrounds both central components of the galaxy. The general morphology suggests a system undergoing a possible major merger or tidal interaction between two galaxies. The light from the individual components appears fairly disturbed. The individual galaxies are round in shape. There are also signs of merging, but there is a notable lack of strong tidal tails or extended features, which might imply a more advanced stage of the merger. 
