  This letter reports on the Galactic stellar structures that appear in the
foreground of our Canada-France-Hawaii-Telecopse/MegaCam survey of the halo of
the Andromeda galaxy. We recover the main sequence and main sequence turn-off
of the Triangulum-Andromeda structure recently found by Majewski and
collaborators at a heliocentric distance of ~20 kpc. The survey also reveals
another less populated main sequence at fainter magnitudes that could
correspond to a more distant stellar structure at ~28 kpc. Both structures are
smoothly distributed over the ~76 sq. deg. covered by the survey although the
closer one shows an increase in density by a factor of ~2 towards the
North-West. The discovery of a stellar structure behind the
Triangulum-Andromeda structure that itself appears behind the low-latitude
stream that surrounds the Galactic disk gives further evidence that the inner
halo of the Milky Way is of a spatially clumpy nature.
