It is visible to the naked eye as a faint, orange-hued star with an apparent visual magnitude of 4.90.

[2] The star is located approximately 430 light years away from the Sun based on parallax.

[1] The radial velocity estimate for this object is poorly constrained, but it appears to be moving closer at the rate of around −5 km/s.

[3] With the supply of hydrogen at its core exhausted, the star has expanded off the main sequence and now has 45[1] times the girth of the Sun.

It is radiating 446[1] times the luminosity of the Sun from its bloated photosphere at an effective temperature of 3,963 K.[1]