The galaxy appears to be undergoing a merger event. There are clear signs of disturbance in its morphology, including what looks to be tidal tails and an irregular overall shape. The galaxy exhibits both smooth and clumpy regions. A fraction of the light appears to be dominated by older stellar populations, indicated by the reddish hue in one area, and a fraction is bluer which is indicative of younger stars. Given the features and merger signatures, the galaxy likely has a low stellar mass and a low star formation rate. The light of the galaxy appears diffuse.
