The galaxy presents as a merging or interacting system, exhibiting a disturbed morphology. There appear to be at least two distinct nuclei, one brighter than the other, indicating potentially two galaxies in the process of merging. The overall structure is irregular, with some evidence of tidal features or debris surrounding the main bodies. The color gradient suggests a range of stellar populations, with bluer regions perhaps indicating areas of ongoing star formation. The galaxy appears relatively compact.
