This galaxy exhibits a moderately disturbed morphology, showing evidence of possible interaction or recent merger activity. The central region is somewhat bright, but the overall structure is diffuse and irregular. There is a suggestion of a disk, but it appears warped or fragmented. Distinct knots of blue light are present throughout, indicating regions of active star formation. These star-forming regions are not uniformly distributed, but concentrated in what appear to be tidal features or disrupted spiral arms. There is evidence of diffuse dust lanes and possible tidal tails, further supporting an interaction or merger scenario. The galaxy is not completely smooth, showing some disturbed features. There also appears to be some disruption from a merger, possibly a minor one. 
