It has a yellow hue but is too dim to be visible to the naked eye with an apparent visual magnitude of 8.26.
[2] The star is located at a distance of approximately 290 light-years from the Sun based on parallax, but is drifting closer with a radial velocity of −30 km/s.
[1] The stellar classification of G3IV/V is consistent with a star that is evolving onto the subgiant branch, having exhausted the supply of hydrogen at its core.
It is roughly four billion years old with a modest projected rotational velocity of 2.3 km/s.
The star is radiating 2.7 times the luminosity of the Sun from its photosphere at an effective temperature of 5,794 K.[3] Using the ESO HARPS instrument, in 2009 HD 191760 was found to have a brown dwarf at least 38 times as massive as Jupiter orbiting at an average distance of 1.35 AU in a period of 506 days.