It has an apparent visual magnitude of 5.47,[2] making it faintly visible to the naked eye from dark suburban skies as a dim, yellow-white hued star.
The system is located 95 light years away from the Sun, based on parallax,[1] but is drifting closer with a radial velocity of −20 km/s.
It is a single-lined spectroscopic binary with an orbital period of 3.128 years and an eccentricity of 0.11.
[3] The primary component has a stellar classification of F8 V or F9 V,[3] indicating it is an F-type main-sequence star.
[3] The system is a source for radio and X-ray emissions, which may be coming from the secondary companion.