The galaxy appears to be undergoing a merger or interaction. Its overall shape is disrupted, showing significant deviations from a regular elliptical or spiral form. There's a noticeable tidal tail or bridge of material extending outwards from the primary body of the galaxy, indicating gravitational interaction with another, possibly unseen, object.

The galaxy exhibits a relatively smooth central region, potentially a bulge, with a color gradient suggesting older stellar populations. There are also bluer regions that imply ongoing or recent star formation. The overall color profile suggests that the galaxy is neither purely quiescent nor vigorously star-forming, but lies somewhere in between.

There is evidence of dust lanes and patches distributed throughout the main galactic body, obscuring some of the starlight. The system is not perfectly symmetrical. It is an interesting system worthy of further observations.
