This galaxy exhibits a disturbed morphology, suggesting ongoing or recent gravitational interactions. The light distribution is not smooth; instead, it appears clumpy and irregular. There is a distinct, brighter region within the galaxy that shows hints of a tidal tail or bridge extending outward. This implies a possible merger event with another galaxy. The color appears bluish, suggestive of a relatively young stellar population and ongoing star formation. However, the morphology is dominated by evidence of disruption.
