橙矮星
The remaining components form a binary star system with an orbital period of 56 years, an angular semimajor axis of , and an eccentricity of 0.13. They have an angular separation of from the primary. The total mass of the pair is and they have a combined visual magnitude of 8.85. The brighter member of this pair is a suspected K-type main-sequence star with a class of K0V.