The galaxy presents as a merging system, dominated by two primary, bright components or galactic nuclei. The interaction appears to be in a late stage, with significant morphological disturbance observed. There is evidence of tidal features, possibly faint tails or bridges of stellar material, extending from the main bodies, although these are subtle. The overall color is relatively uniform, suggesting a well-mixed stellar population or significant dust obscuration. The system's shape is quite irregular, lacking any clear spiral or elliptical structure.
