The galaxy presents a disturbed morphology, indicative of an ongoing or recent interaction. A dominant central region is evident, possibly a bulge component, though its exact nature is obscured by the distortion. Elongated, diffuse tidal features extend from the main body, suggesting gravitational disruption. There is likely ongoing star formation, as evidenced by the bluer color concentrated within certain regions. The overall structure lacks clear spiral arm definition, with evidence of distorted features. The galaxy exhibits a moderate inclination, with a hint of a flattened disk component. Dust lanes are not clearly visible, potentially due to the resolution or inclination.
