The target galaxy appears to be undergoing a significant merger event. The system presents with two distinct, luminous components, each likely representing the core of a progenitor galaxy. One component is more elongated, exhibiting a cigar-like shape. Both components display a central concentration of light, surrounded by a more diffuse halo of bluer emission, potentially indicating ongoing star formation triggered by the interaction. There is evidence of tidal features, suggesting gravitational disturbance as a result of the interaction. The overall morphology is complex and irregular, reflecting the disruptive forces at play during the merger.
