The galaxy appears as a system of merging or interacting components. The overall structure is highly disturbed, indicating significant gravitational interaction. There appear to be at least three distinct concentrations of light. The color suggests an intermediate age stellar population, possibly with some ongoing star formation, but at a relatively low rate. The galaxy is generally rounded in overall shape, though highly distorted with a disturbed morphology. A significant merger event is likely ongoing. The system shows evidence of tidal features and disruptions.
