this star is estimated to be about the same age as the sun, with 83% of the mass of the sun and 82% of the sun's radius. it has not been identified as a member of any moving star groups. this star has displayed unusual emissions of ca ii and is much more x-ray luminous than the sun. it is considered a relatively active star. based on an iron abundance of [fe/h] = -0.02, the metallicity of this star appears to be similar to that of the sun.