This star system belongs to the Zeta Herculis Moving Group of stars that share a common motion through space, suggesting that they have a common origin. In the galactic coordinate system, the components of the space velocity for this system are equal to for ζ1 and for ζ2. They are currently following an orbit through the Milky Way galaxy that has an eccentricity of 0.24. This orbit will carry the system as close as and as far as from the Galactic Center. The inclination of this orbit will carry the stars as much as from the plane of the galactic disk. This likely puts them outside the thick disk population of stars.