The galaxy presents as a somewhat diffuse object, elongated in shape. It exhibits a subtle color gradient, transitioning from a bluer hue at one end to a slightly redder tone towards the opposite end. A substantial portion of the galaxy appears to be characterized by a smoother texture, with some evidence of internal structures. The overall form suggests a disk-like structure, though the orientation and resolution make a definitive classification challenging. There is a hint of possible interaction or disturbance in its morphology, although it does not seem to be undergoing a major merger event. It seems to be low mass and star forming.
