The galaxy appears to be undergoing a major merging event. Two distinct galactic nuclei are visible, indicating at least two progenitor galaxies. The upper nucleus exhibits a bluer color profile compared to the lower nucleus, suggesting a younger stellar population or ongoing star formation. The lower nucleus appears more yellow/red in color, implying an older stellar population and less active star formation.

There is a faint, diffuse envelope of stellar material surrounding both nuclei, exhibiting a tidal stream-like structure, further supporting the merger hypothesis. The morphology indicates significant gravitational interaction and disruption of the original galaxy structures. The system appears relatively compact, suggesting that the merger is in its later stages. Overall, it seems to be an actively evolving system.
