  NGC 6240 is a rare object in the local universe: an active merger remnant
viewed at the point of merging where two active galactic nuclei are visible. We
present IRAC data of this object, providing high sensitivity maps of the
stellar and PAH distribution in this complicated system. We use photometry to
analyze the variation in these distributions with radius and provide an SED in
the four IRAC bands: 3.6 microns, 4.5 microns, 5.8 microns and 8.0 microns. We
fit the radial profiles of the 3.6 micron band to r^.25 and exponential
profiles to evaluate the structure of the remnant. Finally, we compare the IRAC
images with multi-wavelength data and examine how outflows in the X-ray, Halpha
and CO correlate with 8 micron emission. The results support the general
picture of NGC 6240 as a system experiencing a major merger and transitioning
from a disk galaxy to a spheroid. The sensitivity of IRAC to low surface
brightness mid-infrared features provides detailed information on the extended
distributions of stars and dust in this rare system.
