The galaxy presents with an irregular morphology. It lacks a clearly defined nucleus or spiral arm structure. There is an apparent tidal tail, which seems to extend from the main body, suggesting an ongoing or recent gravitational interaction or merger. The galaxy exhibits a clumpy structure. The color distribution is not uniform; a greenish-blue hue is most apparent, but there are areas of redder coloration interspersed throughout the galaxy. These color variations could indicate differing stellar populations or regions of active star formation. A fraction of the light appears to be highly redshifted. The galaxy displays a somewhat diffuse and disturbed morphology. Overall, the morphology suggests a system undergoing significant dynamical processes.
