[5] It is visible to the naked eye as a faint, orange-hued star with an apparent visual magnitude of 4.97.
[2] This object is drifting closer to the Earth with a heliocentric radial velocity of −22 km/s.
Having exhausted the supply of hydrogen at its core, this star has expanded to 26 times the Sun's radius.
[1] Within the margin of error it has near-solar abundances of iron,[2] suggesting a Sun–like metallicity.
The star is radiating 214[1] times the luminosity of the Sun from its swollen photosphere at an effective temperature of 4,332 K.[1]