  Recently there has been a hint of a gamma-ray line at 130 GeV originated from
the galactic centre after the analysis of the Fermi-LAT satellite data. Being
monochromatic in nature, it rules out the possibility of having its
astrophysical origin and there has been a speculation that this line could be
originated from dark matter annihilation. In this work, we propose a two
component dark matter scenario where an extension of the Standard model by an
inert Higgs doublet and a gauge singlet scalar concocted with $\rm {Z_2 \times
Z^{\prime}_2}$ symmetry, is considered. We find that our scenario can not only
explain the 130 GeV gamma-ray line through dark matter annihilation but also
produce the correct dark matter relic density. We have used the Standard Model
Higgs mass around 125 GeV as intimated by the LHC data..
