It is visible to the naked eye as a faint, orange-hued point of light with an apparent visual magnitude of 4.91.

[2] The system is located approximately 350 light years away from the Sun based on parallax,[1] and is drifting further away with a mean radial velocity of +30 km/s.

[4] The system has a relatively high proper motion, traversing the celestial sphere at the rate of 0.186 arc seconds per annum.

It is a single-lined spectroscopic binary system with an orbital period of 6.86 years and an eccentricity of 0.38.

Having exhausted the supply of hydrogen at its core, the star has expanded to 22[1] times the Sun's radius.