The galaxy appears to be undergoing a major merger. Two distinct galactic nuclei are observed, suggesting two separate galaxies are in the process of gravitationally interacting. The southern nucleus appears slightly elongated and has a more defined structure, surrounded by a less-defined halo of light. The northern nucleus is more compact and appears more diffuse.

Significant tidal features, likely tidal tails or bridges, connect the two nuclei. Light from this system exhibits a bluer hue than the surrounding area, potentially indicating a high star formation rate triggered by the merger. The overall morphology is disturbed, lacking a clear disk or elliptical shape, which further supports the classification of a merging system. There may be another small object to the north of the top galaxy, but more data is needed.
