The galaxy appears to be an interacting system, possibly in the later stages of a merger. The primary body of the galaxy exhibits a smooth, somewhat rounded morphology, though with some subtle irregularities. There is evidence of significant tidal disruption. The galaxy is not completely spheroidal as there are clear asymmetries and extended, faint structures, possibly tidal tails or disrupted spiral arms. There is a definite blue-shifted light distribution. The overall color suggests a moderate amount of on-going or recent star formation. This system seems to be actively evolving, likely driven by the gravitational interaction and merging process.
