Parallax measurements made during the Gaia mission make this system to be approximately 93.9 light-years (28.8 parsecs) from Earth.

Its apparent visual magnitude is +4.83,[2] which makes it bright enough to be seen with the naked eye.

[4] The IV luminosity class indicates that it is probably a subgiant star that is in the process of evolving away from the main sequence as the supply of hydrogen at its core depletes.

[10] At the system's estimated distance this yields a size of about 2.2 times that of the Sun.

[6] It is emitting about seven times solar luminosity from its outer atmosphere at an effective temperature of 6,628 K.[7] This heat gives it the yellow-white-hued glow of an F-type star.