The galaxy appears to be an ongoing merger of two distinct galactic systems. Each component exhibits a generally smooth morphology. The primary galaxy displays a redder hue, suggesting an older stellar population or significant dust obscuration. The secondary galaxy is characterized by a bluer color, potentially indicative of ongoing star formation. There are morphological indications of tidal interactions between the two galaxies with evidence of disruption of the galactic structure, suggesting a merger in progress. The overall estimated stellar mass suggests a relatively large system. Relatively low star-formation rates suggest that this might be in the later stages of its evolution.
