The galaxy presents a disturbed morphology, possibly indicative of an ongoing or recent merger event. The structure exhibits features of a disk galaxy, although significantly perturbed.

A central bulge is evident, surrounded by a complex system. There are two apparent cores, with significant light emitted from each. Tidal tails appear to be present, suggesting gravitational interaction.

The overall color suggests a mix of stellar populations. Regions display bluer colors, indicating recent star formation, while other areas appear redder, potentially signifying older stellar populations. The luminosity is relatively high, hinting at a substantial stellar mass. Overall, the galaxy presents a unique and complex morphology, meriting further investigation.
