This galaxy appears to be undergoing a significant merger event. Two distinct luminous regions are visible. The larger region exhibits a smoother, more diffuse morphology, with a centrally concentrated luminosity profile. It displays a bluer color, suggestive of a younger stellar population and ongoing star formation activity. The smaller region presents a yellower color, which may indicate an older stellar population. This region appears more compact. The overall shape of the merging system is moderately rounded.
