The galaxy appears to be undergoing a major merger. Two distinct nuclei are visible, exhibiting reddish hues which might indicate older stellar populations or significant dust obscuration. A diffuse, greenish envelope surrounds both nuclei, likely representing tidal debris and newly formed stars triggered by the interaction. The overall morphology is highly disturbed, with indications of extended tidal tails or bridges suggestive of strong gravitational interaction. The system exhibits a generally amorphous shape, far from a regular spiral or elliptical form. The smoothness of the central regions suggest a lack of distinct spiral arm structures, further supporting the hypothesis of an ongoing merger event. Star formation appears to be present in some regions of the galaxy.
