This galaxy exhibits a morphology suggestive of a late-stage merger. A prominent tidal tail extends from the main body of the galaxy, indicating a gravitational interaction. The color gradient along the galaxy appears to shift from bluer hues in what may be the primary nucleus to redder hues in the secondary nucleus and tidal tail.

There are hints of internal structures in the galaxy, but they are not well-defined. The merging galaxy is actively forming stars in the blue region of the primary nucleus, indicating gas-rich processes are occurring as a result of the collision. The mass is significant suggesting this is an interaction between two large galaxies.

The system is not perfectly relaxed, with an irregular shape indicative of ongoing dynamic processes. The overall appearance is dominated by the ongoing interaction and resulting disturbances.
