This galaxy appears to be a single system undergoing significant interaction or a full-blown merger with at least one other galaxy, possibly two, though that is less clear. The morphology of the primary galaxy appears to be disturbed; there is no clear spiral structure, and the overall form suggests tidal distortion. One of the components is compact and bright, while the rest of the galaxy is more diffuse. The system's red color suggests a population of older stars. Given its luminosity, the galaxy likely has a relatively high stellar mass and a low rate of ongoing star formation. There is some irregularity in the shape, possibly indicative of a late-stage merger.
