The observed galaxy presents a somewhat irregular morphology. It appears to be undergoing a significant interaction or merging event. There are two particularly prominent, bright regions, one showing a reddened color. A more diffuse, bluer component surrounds the brighter regions, potentially representing tidal debris or disturbed disk material. There is evidence suggesting potential minor and major disturbances, in the form of distortions. The overall structure lacks a well-defined disk or spiral arm pattern, suggesting a complex and dynamic system. The galaxy shows both smooth and featured components.
