One of the most exciting things about this discovery is that because Barnard's star is so close, the planet should have a maximum angular separation of 0.22 arcseconds. Directly imaging the planet in reflected light from the star [1] will be no problem for next generation telescopes in terms of resolution and sensitivity -- telescopes like the 30 meter class facilities being built now or a hypothetical ~10 meter space telescope called "LUVOIR". Current cutting edge instruments like the Gemini Planet Imager (GPI) can already get to about 0.2 arcsec resolution, but it operates in the infrared and can only detect down to about a Jupiter-mass depending on how hot the planet is. The really exciting thing about imaging a planet in reflected light is that you can study the composition of the atmosphere in much greater detail than current methods [2]. This is likely the first system that astronomer's will target when they seek to make direct observations of a rocky planet's atmosphere outside of our Solar System.
[1] Ss opposed to the thermal infrared, which works best for young planets which have substantial residual heat from their formation.
[2] Such as when an exoplanet transits in front of it's host star, the atmosphere will absorb some light. However it appears this technique is only sensitive to the very thin upper parts of the atmosphere, and we don't learn much about the rest.