Just looking at it's characterstics.....it is 1.6 earth radius's.....so likely enough mass to retain an atmosphere. Also it's orbital period is only 17.9 days.
The way the winds work is by convection currents, and if there is life, it would be along the transition area between the two distinct sides of the planet. There will be the life supporting temperatures and conditions.
Also, it is worth pointing out that the tidal lock of its orbit is a theory due to it's proximity to it's parent star.
Can't just base a planets ability to retain an atmosphere on its mass. Sure, its a factor, but so is proximity to the star, heat output, spectral output and its affect on the specific molecules making the atmosphere.
As for the convection currents, sure I'm in agreement there, but factor in the losses as the gases condense on the cold side, which will drop atmospheric pressure so that any returning gases will be less in volume than the gases that are being supplied. Eventually what was the atmosphere could well be transported to the cold side of the planet for deposition, leaving the sunny side greatly thinned. I think the chances of a life supporting environment in the transition zone would be minimal.