The galaxy presents as a system undergoing significant gravitational interaction. It appears to be in the late stages of a merger event, possibly involving two or more galaxies. Evident are strong tidal features, including extended tails and distorted spiral arm structures. The central region exhibits a complex morphology, with indications of intense star formation activity, especially prominent in bluer wavelengths. The overall color gradient suggests a relatively young stellar population. This galaxy has a relatively high mass estimate, but low star formation rate. 

The galaxy's redshift indicates a substantial cosmological distance. The galaxy is most likely an interacting system with merging galaxies, which agrees with the Galaxy Zoo data.
