[2] Based upon an annual parallax shift of 27.80[1] mas as seen from Earth, it is located around 136 parsecs (440 ly) distant from the Sun.
The secondary, component B, is a chemically peculiar A-type main sequence star with a class of A5 Vp[4] and an estimated mass 2.10 times that of the Sun.
[12] The outer member, component C, has an orbital period of around half a million years.
[12] As of 2007, it had an angular separation of 115.8 arc seconds along a position angle of 248° from the primary.
[3] It is an F-type main sequence star with a classification of F5 V and an estimated 1.29 times the Sun's mass.