This galaxy exhibits a non-regular morphology, indicating a possible interaction or merger event. There appear to be two distinct, high-intensity central luminous regions or galactic cores, suggesting either an ongoing merger of two galaxies, or significant tidal disruption within a single galaxy. The overall shape is somewhat rounded, though the tidal features distort this overall roundness. Diffuse, fainter light surrounds the central regions, forming an envelope with irregular extensions, potentially indicative of tidal tails resulting from gravitational interactions. There is also some evidence of disk-like qualities within the morphology. Light appears predominantly in the green channel and fainter in the blue channel; the redshift could be significant enough to move light from the red channel to the green, and light from the green to the blue, if the object has a high redshift.
