The galaxy appears to be undergoing a merger event. Two distinct galactic nuclei are visible, each embedded within a diffuse, elongated body of stars. The primary galaxy displays a smoother, more concentrated light distribution, suggesting an older stellar population. The secondary galaxy appears less defined and slightly redder in color, possibly indicating ongoing star formation or a dustier environment. There is a notable tidal tail present, extending from the interacting system, which is indicative of gravitational disruption caused by the ongoing merger. The overall morphology of the system is disturbed, lacking the well-defined spiral arms or elliptical shape often observed in isolated galaxies.
