Low mass stars (and this one is very low mass) are dim, so the habitable zone is very close, so tidal effects of the star on the planet are large*, so under normal circumstances the planet will tidally lock to the star, which is not friendly to life. (Although I wouldn't go so far as to say life is impossible on a tidally locked world.)
If the planet has a large enough moon, it will lock to the moon instead, and avoid the star tidal lock (at least for a while.) So I imagine a planet and moon locked to each other and in close orbit around the star. In this case, what will happen to the planet/moon orbit as it gets perturbed by the stellar tides? Will it remain stable, or has the moon only bought me temporary reprieve from stellar tidal lock?
* Back of envelope tidal calculation:
Luminosity of star L proportional to mass of star M to 4th power (roughly)
Goldilocks orbital radius R proportional to sqrt(L), i.e. R propto M^2
Tidal strength T propto M/R^3 (it is derivative of M/R^2), so T propto M/M^6 = 1/M^5. (It is the 1/R^3 which allows a moon to out-tide the star, despite being very much less massive.)
News says this star is 2000 times fainter than the sun, so about 0.15 solar masses
So tidal effects of star on habitable planets is about 13,000 times greater than tidal effect of sun on earth.
The tidal effect of the sun on the earth are small but noticeable - it causes the difference between spring and neap tides.