  The viability of neutralino dark matter as an explanation of the 130 GeV
gamma ray signal from the Galactic Center recently observed by the Fermi Large
Area Telescope is examined. It is found that the signal can be compatible with
a sharp feature from internal bremsstrahlung from a mostly bino dark matter
particle of mass around 145 GeV, augmented by a contribution from annihilation
into gamma+Z via a small wino admixture. This scenario circumvents the
problematic overproduction of lower energy continuum photons that plague line
interpretations of this signal. Sleptons approximately degenerate in mass with
the neutralino are required to enhance the internal bremsstrahlung feature.
