The object appears as a pair of distinct, roughly symmetrical luminous regions. These regions display diffuse, albeit somewhat ill-defined, boundaries with a noticeable blue-shifted halo around each one. The red and green light is more focused in the central part of each luminous region, indicating perhaps older stellar populations, dust obscuration, or differential reddening. 

There is faint evidence of a bridge-like connection between the two luminous regions, but this is not sharply defined. There is no clearly defined nucleus or bulge within the regions. The morphology suggests the possibility of a galaxy undergoing an ongoing major merger event. Evidence for tidal features or significant disturbances appears to be present, although they are subtle. Overall, the galaxy exhibits a relatively small apparent size.
