 The secondary component has about 6–13% of the primary's mass and may have a stellar classification in the range from A6 V to K1 V. There may be a third component to this system with an orbital period of roughly 9,428 days (25.8 years), although this has not been conclusively demonstrated.If this component exists, it would have about 51–139% of the primary's mass.This high level of uncertainty is because the inclination of the orbit is not known.