The galaxy exhibits a disturbed morphology, potentially indicative of an ongoing or recent merger event. Multiple luminous clumps are visible, suggesting regions of intense star formation activity. These clumps are distributed across the galaxy's main body, lacking a clear central concentration. Some diffuse light is visible, extending beyond the denser regions, hinting at tidal interactions. The overall color appears blueish, which supports the presence of young, hot stars associated with active star formation. There may be some spiral arms, but the merger makes them difficult to clearly distinguish. A small bulge may be present.