The galaxy exhibits a disturbed morphology, indicative of an ongoing or recent interaction. It appears to be composed of at least two distinct luminous components, possibly individual galaxies in the process of merging. The overall structure lacks a clear spiral or elliptical shape. The brighter, central region shows signs of tidal disruption. There is no clear indication of a dominant bulge or disk. Overall color is on the bluer side, suggesting the presence of stellar formation regions. There appears to be a tidal tail.
