The galaxy exhibits a disturbed morphology, suggestive of an ongoing or recent interaction. Two distinct, bright nuclei are visible, indicating the presence of at least two galactic components. These components appear to be connected by faint, diffuse material. The overall shape is irregular, with no clear spiral arm structure discernible. There is a strong blue color near the center of each of the galactic nuclei. Red light is visible on the outskirts of the galaxies, and some merging of the colors is apparent. The galaxy shows signs of disturbance but no clear major disturbance.