  We study a three loop induced radiative neutrino model with global $U(1)$
symmetry at TeV scale, in which we consider two component dark matter
particles. We discuss the possibility to explain the X-ray line signal at about
3.55 keV recently reported by XMN-Newton X-ray observatory using data of
various galaxy clusters and Andromeda galaxy. Subsequently, we also discuss to
show that sizable muon anomalous magnetic moment, a discrepancy of the
effective number of neutrino species $\Delta N_{\rm eff}\approx$ 0.39, and
scattering cross section detected by direct detection searches can be derived.
