[9] It is a probable member of the open cluster NGC 6882.
[4] This object is visible to the naked eye as a faint, orange-hued star with an apparent visual magnitude of 5.40.
[2] It is moving closer to the Earth with a heliocentric radial velocity of −19 km/s.
[4] This is an aging giant star with a stellar classification of K2 IIIa,[3] having already consumed the hydrogen at its core and evolved away from the main sequence.
The star is radiating 2,889[1] times the Sun's luminosity from its enlarged photosphere at an effective temperature of 4,200 K.[7]