The galaxy appears to be in a late-stage merger, exhibiting a complex morphology. There are two distinct brightness peaks. The peak on the right is brighter and has a blue-green hue. The other peak on the left has an orange-red hue. A faint bridge of light seems to connect them. The overall shape of the galaxy is somewhat rounded, but with clear disturbances in its structure suggesting ongoing tidal interactions. The color variations suggest differential star formation rates or dust content within the merging components.
