It has an apparent visual magnitude of 3.75,[2] which is sufficiently bright to allow it to be viewed with the naked eye.

Based upon an annual parallax shift of 30.33 mas as seen from Earth, its distance can be estimated as 107.5 light years from the Sun.

The star is moving away from the Sun with a radial velocity of +27 km/s.

It is a red clump star,[3] which means it is on the horizontal branch and is generating energy through helium fusion at its core.

[7] It is radiating about 41 times the Sun's luminosity from its enlarged photosphere at an effective temperature of 4,546 K.[7]