The galaxy appears to be undergoing a significant merger event. There are two distinct, luminous components visible. One component exhibits a bluish-white color, indicative of a region with ongoing star formation. The second component appears more reddish-yellow in color, suggesting an older stellar population. The morphology of the interacting system is highly disturbed, with potential tidal features or extended plumes of material. There is a reasonable fraction of the light coming from older, smoother populations.
