The galaxy presents as a system undergoing significant interaction or merging. It appears to consist of at least two primary components, possibly galactic nuclei, evidenced by the irregular, disturbed morphology and the extended, diffuse tidal features. The galaxy is dominated by bluer light, suggesting active star formation, particularly in the areas of highest luminosity. There is a hint of redder light on one side of the galaxy. The system lacks a well-defined, organized spiral structure or a smooth elliptical profile. The overall shape is highly distorted, with noticeable asymmetries in the luminosity distribution. The merging process appears to be well underway, with a high degree of disruption to the original galactic forms.
