The galaxy presents as a system undergoing a significant merger event. There are at least three distinct components visible, exhibiting varying colors. One component appears to have a reddish hue, suggesting an older stellar population or significant dust obscuration. Another component shows a bluer color, indicative of ongoing star formation activity. The third component is somewhat dimmer than the others, with no strong color distinction. The overall morphology is disturbed and irregular, lacking a defined spiral or elliptical structure. The system appears to be relatively compact, with a notable degree of interaction between the components, reinforcing the interpretation of an ongoing merger.
