The galaxy appears to be an interacting system, possibly in the late stages of a merger. Two distinct nuclei are visible, suggesting the remnants of two progenitor galaxies. The northern nucleus exhibits a more diffuse, rounded morphology, while the southern nucleus is slightly more elongated. A faint tidal bridge or tail seems to connect the two nuclei. The overall color is somewhat green, hinting at ongoing star formation. There is a relatively smooth halo surrounding the main components, indicating previous interactions have begun to smooth. Signs of significant disturbance in the overall structure indicate the influence of gravitational forces during the merging process.
