[2] Based upon an annual parallax shift of 26.2 mas, the system is located around 124.5 light years away.
The authors of the study estimated a class of K2 V, based upon a visual magnitude difference of 2.3±0.5.
[6] Subsequent observations using adaptive options did not spot this companion and it was concluded this was a false detection.
This red dwarf star has 0.33–0.45 times the mass of the Sun and is orbiting with a semimajor axis of 35–60 AU.
This object orbits at 3 AU away from the primary star with a period of 1,634 days and an eccentricity of 0.7.