The galaxy presents as a somewhat diffuse object, exhibiting an irregular morphology. It appears to be undergoing a significant interaction or merger event. Multiple distinct luminous regions are visible, suggesting the presence of separate galactic nuclei or areas of intense star formation triggered by the interaction. The overall color is yellowish, which could indicate an older stellar population, although the interaction may also be inducing localized regions of younger, bluer stars that are not readily discernible at this resolution. There appears to be limited evidence of a well-defined disk structure; instead, the light distribution is more chaotic and disturbed. The merging process might be disrupting any pre-existing spiral arms or disk features. The overall appearance suggests a system where gravitational interactions are currently playing a dominant role in shaping the galaxy's structure and evolution.
