  A map of the projected density of the old stellar population of the Galactic
Bulge region is reconstructed using 2MASS data. By making a combination of the
H and K photometric bands, it is possible to overcome the effect of reddening,
and thus penetrate the inner structure of the Galactic Bulge. The main
structure in the map corresponds to the well documented peanut shaped bar which
is formed by the inner parts of the Galactic disk as a result of dynamical
instabilities. As suggested by numerical simulations, the projected Z profile
of the bar, has an almost exponential shape. After subtracting the exponential
profile associated with the bar, a large residual appear near the Galactic
Center. This residual is elongated and asymmetrical, which suggest a bar
structure. Thus we arrive at the conclusion that in addition to the main bar a
smaller bar with a different orientation may exist in the central region of the
Milky Way. This finding makes the Milky Way very similar to a large number of
barred spiral Galaxies which show as well a smaller bar in their central
regions.
