 The distance to this system is around 367 light years, as determined from an annual parallax shift of 8.89 mas.Judging by its motion through space and physical properties, this system is a member of the Upper Centaurus Lupus group of the Scorpius-Centaurus Association.It is double-lined spectroscopic binary with an orbital period of just 3.3 days and an eccentricity of 0.28.