This galaxy presents a disturbed morphology, exhibiting features suggesting an ongoing or recent merger event. There are clear asymmetries and irregularities in the overall structure, with noticeable clumpy regions indicative of possible tidal tails or disrupted arms. The central region appears somewhat diffuse, lacking a well-defined nucleus or bulge. A bluish hue permeates the galaxy, implying the presence of young, hot stars and ongoing star formation. The galaxy shows evidence of significant interaction and disturbance, likely driving the observed star formation activity.
