The galaxy appears to be an interacting system, possibly in the late stages of a merger. There is a clear disturbance of the morphology, with tidal features evident in the form of faint extensions or plumes emanating from the main bodies. 

The galaxy exhibits at least two distinct nuclei or regions of high luminosity, suggesting the presence of two progenitor galaxies. One nucleus is bright and relatively unresolved in this image, while the other is less luminous and appears more diffuse, with a slightly bluer color. There appears to be considerable star formation occurring, indicated by the presence of blue regions. A redder component may indicate an older stellar population, possibly within the bulge of a progenitor galaxy. 

The overall shape is irregular, lacking the defined spiral arms or elliptical structure. There is a suggestion of a disk-like component, but it is heavily warped and disrupted, consistent with the ongoing interaction. The system's spatial extent is significant, indicating a developed merging event. Evidence of dust lanes or obscuration may be present but cannot be definitively determined from this image.
