I have addressed in my answer to your last question that you cannot simply use the luminosity to calculate an apparent visible magnitude, because at 2895 K most of this star's emission is not in visible wavelengths (rather, it's in infrared).
All of the other answers are overestimates to some degree. Subtracting about 3.5 magnitudes of difference between bolometric and V-band (which is the set of wavelengths human eyes are most sensitive to, so it's a proxy for the light humans will pick up on), we get an apparent magnitude of about -10.5. See my previous answer for the source on that. This is about six times fainter than the full moon here on Earth, and very roughly comparable to the brightness of a half moon (though sources disagree on whether this might be more like 10 or 12... call it a slightly gibbous moon, then.)
Needless to say, you may be able to use the light of a half moon to navigate at night, but in a rural area you will very much find it dark.