The galaxy appears to be in a late-stage merger. The morphology is significantly disturbed, exhibiting a highly irregular shape. Two distinct, bright nuclei are visible, suggesting the cores of the progenitor galaxies have not yet coalesced. The overall color is reddish, indicative of an older stellar population and/or significant dust obscuration. There is evidence of tidal features, possibly faint streams or tails, extending outward from the main body of the galaxy. These features are very subtle, suggesting they are either faint or obscured. Star formation appears to be relatively low, based on the color, which indicates a low fraction of young, blue stars. 
