The distance to this star is 102 light years, but it is drifting closer to the Sun with a radial velocity of −20 km/s.
[2] The star has a relatively large proper motion, traversing the celestial sphere at an angular rate of 0.289 arcsec yr−1.
[8] This object is a solar analog with a stellar classification of G5 V;[3] a G-type main-sequence star like the Sun that is generating energy through core hydrogen fusion.
It is radiating 1.5 times the Sun's luminosity from its photosphere at an effective temperature of 5,836 K.[5] In 2020, a stellar companion was identified using high-contrast imaging.
They propose this is a faint red dwarf with a class of M6 or later and a visual magnitude difference of 7.9 or more compared to the primary.