The galaxy appears to be a gravitationally interacting system. There is a central, fairly concentrated body with a smooth appearance. Adjacent to this central body is another distinct, but smaller, bright region. This neighboring region exhibits a bluer color than the central body. There is evidence of tidal features or diffuse extensions emanating from the central body that suggest a merger event may be occurring. Overall, it seems to be a fairly massive system with intermediate star formation activity, showing signs of possible disturbance in its morphology.
