The galaxy appears to be undergoing a merger. The system displays a complex morphology with two distinct, bright nuclei. One nucleus exhibits a reddish hue, suggesting a region of older stellar populations and/or significant dust obscuration. The other nucleus is yellower, indicating a mix of stellar populations. Evidence of tidal disturbances is observed with diffuse extended features suggesting interactions and gravitational disruption of the galactic structure. There are subtle indications of arm-like structures or extended features that may have been disrupted and stretched by the interaction. The overall shape of the system appears moderately round, but this assessment is limited due to the ongoing merger. Star formation rates are low within this system.