The galaxy appears to be in a late-stage merger or interaction with at least one other galaxy or large clump of stellar material. The primary body exhibits a generally smooth morphology but with clear signs of tidal disruption. There is an elongated tidal tail or bridge extending outwards, suggesting a gravitational interaction with the other nearby clump. The main body has a fairly bright yellowish-orange core and then becomes more blue tinged in its outer regions. The overall shape is somewhat irregular, deviating significantly from a perfect ellipse or disk-like structure. The merging or interacting component has a more clumpy and irregular appearance, with a distinct bluish color. Overall this system demonstrates significant levels of disturbance likely induced by the gravitational interaction currently in progress.
