The galaxy presents a morphology suggestive of an ongoing interaction or merger event. The main body appears diffuse, with a somewhat elongated structure oriented in a roughly vertical direction. A noticeable feature is the presence of what appear to be tidal tails extending outward from the main galactic body, these tails are characterized by a bluer color, potentially indicating regions of active star formation fueled by the interaction. There is a possible disk structure in the lower portion of the galaxy that is bluer than the core. The overall light distribution is irregular, lacking a clearly defined nucleus or spiral arms. Based on its asymmetrical shape and extended features, this galaxy is likely undergoing gravitational disturbances.
