  The Milky Way is the only galaxy for which we can resolve individual stars at
all evolutionary phases, from the Galactic center to the outskirt. The last
decade, thanks to the advent of near IR detectors and 8 meter class telescopes,
has seen a great progress in the understanding of the Milky Way central region:
the bulge. Here we review the most recent results regarding the bulge
structure, age, kinematics and chemical composition. These results have
profound implications for the formation and evolution of the Milky Way and of
galaxies in general. This paper provides a summary on our current understanding
of the Milky Way bulge, intended mainly for workers on other fields.
