It is a fifth magnitude star, which means it is bright enough to be faintly visible to the naked eye.

[2] Based upon an annual parallax shift of just 3.13 mas as seen from Earth,[1] this star is located roughly 770 light years from the Sun, give or take a 40 light year margin of error.

[5] This is an evolved G-type bright giant star with a stellar classification of G6.5 IIb.

[11] This s-process element may have been accreted from a now white dwarf companion during a previous stage of its evolution.

The star is radiating 1,087 times the Sun's luminosity from its enlarged photosphere at an effective temperature of about 4,916 K.[7]