[3] With an annual parallax shift of 10.54 mas,[2] it is roughly 310 light years from the Sun.

At that distance, the visual magnitude of this system is diminished by an extinction factor of 0.22 due to interstellar dust.

This is a single-lined spectroscopic binary star system with an orbital period of 14.48 days and an eccentricity of 0.27.

[8] The visible component is a B-type main sequence star with a stellar classification of B3 V.[4] It is a helium-weak chemically peculiar star[13] and a rotating ellipsoidal variable.

[9] This is a candidate Vega-like star, meaning that it shows an infrared excess characteristic of a circumstellar debris disk.