This galaxy appears to be undergoing a major merger. It presents a disturbed morphology, indicative of strong gravitational interactions. Two distinct, bright nuclei are visible, suggesting the presence of two progenitor galaxies in the process of coalescence. The overall shape is irregular, deviating significantly from a smooth, elliptical structure or a well-defined spiral disk.

The light distribution is concentrated around the two nuclei, with fainter, diffuse emission extending outwards. There is a noticeable tidal feature, possibly a faint bridge or tail, indicating material being stripped from the interacting galaxies. The overall color is relatively red, suggesting a population of older stars and/or significant dust obscuration.

The image suggests an ongoing dynamic process, where the original structures of the galaxies are being disrupted and reshaped by the merger. Star formation rate is probably low, with the galaxy dominated by old stars.
