The galaxy appears to be a late-stage merger of two distinct galactic nuclei or two separate galaxies. The morphology suggests a complex, disrupted structure, possibly due to tidal interactions during the merging process. The overall color of the galaxy is yellowish, hinting at an older stellar population. However, bluer regions might indicate ongoing or recent star formation activity. It is relatively compact, approximately 10 kpc in size, with a generally smooth appearance. However, there seems to be some disturbances present, hinting at an evolving system.
