The object appears to be a galaxy undergoing a merger. The system presents with two distinct components: A dominant, relatively smooth component and a secondary component with a more irregular shape. The primary component exhibits a fairly round morphology, with light primarily at the bluer end of the spectrum. The secondary component is smaller, more diffuse, and shows an orange hue, possibly indicating an older stellar population or the presence of dust. The two components are in close proximity, suggesting a strong gravitational interaction. There may be signs of tidal disturbances in the overall structure.
