The galaxy presents a complex morphology indicative of a system undergoing interaction or merger. There are two distinct, bright nuclei, one appearing more diffuse and slightly redder than the other. These nuclei are likely the cores of the original galaxies involved in the interaction. A faint bridge of material seems to connect the two nuclei, suggesting tidal forces are at play. The overall color gradient is reddish, indicating a population of older stars or significant dust obscuration. There are some signs of disturbance in its shape. 
