The two members of this system orbit each other with a period of 3.80 years and an eccentricity of 0.017.
Both components of the system are F-type main sequence stars with a stellar classification of F7 V.[3] The pair have an apparent visual magnitude of 5.75,[2] which is just bright enough to be faintly visible to the naked eye.
Based upon an annual parallax shift of 28.79 mas,[1] the distance to this system is approximately 113 light-years (35 parsecs).
The system is located near the ecliptic, so it is subject to occultation by the Moon.
This binary or multiple star system–related article is a stub.