The galaxy in the image presents as a complex system, likely undergoing or having recently undergone a merger. A significant tidal tail or stream of stellar material extends outwards, indicating gravitational interaction with a nearby galaxy. The main body of the galaxy appears to be elongated, suggesting some disturbance to its overall morphology. There is evidence of possible active star formation within both galactic nuclei, one of which is more compact than the other. The other appears to have an older stellar population. The overall color gradient suggests a range of stellar populations present within the galaxy. There is a significant dust lane, which could be from one of the galaxies being pulled into the larger system.
