The galaxy exhibits a complex morphology, appearing to be undergoing a significant interaction or merger event. It is composed of at least two distinct luminous components. The northern component displays a bluer hue, suggesting a younger stellar population, while the southern component shows a more yellow and white coloration, potentially indicating an older stellar population.

There is evidence of tidal features or disturbed morphology extending from the main body of the galaxy. The overall structure indicates a system that is not relaxed or in equilibrium, suggesting ongoing gravitational interactions and possible star formation activity. A moderate degree of asymmetry is present in its overall shape.
