The galaxy presents an irregular morphology, seemingly undergoing a major merger event or interaction. Two distinct nuclei are visible, each exhibiting a concentrated, yellowish-white luminosity, potentially indicating older stellar populations or active galactic nuclei. Faint, diffuse blue light surrounds the nuclei, possibly representing areas of recent star formation induced by the interaction. The overall structure lacks a defined spiral or elliptical shape, which supports the hypothesis of a disturbed system. The galaxy appears relatively smooth in some regions, but there are noticeable disturbances, possibly due to tidal forces. The general shape is somewhat elongated, hinting at ongoing gravitational interactions.
