11 Leonis Minoris is a binary star[3] located 36.64 light years away from Earth,[2] in the northern constellation of Leo Minor.

[12] It is visible to the naked eye as a dim, yellow-hued star with an apparent visual magnitude of 5.54.

[6] It has a relatively high proper motion, traversing the celestial sphere at the rate of 0.764 arc seconds per annum.

[8] This is an RS Canum Venaticorum variable star with its luminosity varying by 0.033 magnitudes over a period of 18 days.

[1] Compared to the Sun, it has more than double the abundance of elements more massive than helium—what astronomers term the star's metallicity.