The galaxy exhibits a complex morphology, appearing to be in a late stage of a major merger event. Two distinct luminous nuclei are visible, suggesting the remnants of two progenitor galaxies. A tidal tail emanates from the lower nucleus, curving upwards towards the upper nucleus, indicating significant gravitational interaction and disruption. The color gradients suggest varying stellar populations, with the nuclei showing a yellowish hue, potentially indicating older stellar populations, while the connecting regions show bluer colors, perhaps suggesting more recent star formation triggered by the merger. The overall structure appears highly irregular, deviating significantly from a typical spiral or elliptical morphology.
