The object is a binary system at a distance of around 50 parsecs from the sun. The primary component is a G2VI star. The secondary component remains unidentified. The V magnitude appears variable with a range of at least 0.12 magnitudes.
Colour indices appear stable.
The system has a radial velocity of , an orbital period of 29.9 days and an eccentricity of 0.41. The total space velocity with respect to the galactic center is 340 and the object approaches escape velocity.