The galaxy appears to be in the late stages of a merger. Two distinct, luminous galactic nuclei are visible, suggesting the progenitors have not fully coalesced. The upper nucleus displays a whiter hue, indicative of potentially older stellar populations, or less dust obscuration. The lower nucleus exhibits a yellower color, possibly indicating the presence of younger stars, ongoing star formation, or significant dust content. A faint tidal tail or bridge of material seems to connect the two nuclei, supporting the merger hypothesis, though the exact morphology is difficult to discern given the image resolution. Overall, the galaxy's shape is irregular and disturbed, consistent with the gravitational interactions inherent in a merging system. Star formation rate appears low and total mass is quite high. The system presents a rounded shape. 
