It is faintly visible to the naked eye with an apparent visual magnitude of +5.31.
[2] Based upon an annual parallax shift of 28.27 mas as seen from the Earth,[1] it is 115 light years from the Sun.
The star is moving away from the Sun with a radial velocity of +4.6 km/s.
[4] This is an F-type main-sequence star with a stellar classification of F5 V.[3] This indicates that, at the age of 2.2[6] billion years, it is still generating energy through hydrogen fusion at its core.
It is radiating 7.5[7] times the Sun's luminosity from its photosphere at an effective temperature of 6,471 K.[6] The star has an estimated 1.4[6] times the mass of the Sun and is spinning with a moderately high projected rotational velocity of 44.4 km/s.