In the present work, we adopt a relativistic constituent quark model to depict the charmed strange meson spectroscopy, in which D_{s0}(2317) and D_{s1}(2460) are considered as the 1^3P_0 and 1P_1^prime charmed strange mesons, respectively. By using the wave function obtained from the relativistic quark model, we further investigate the electric transitions between charmed strange mesons. We find the long wave length approximation is reasonable for the charmed strange meson radiative decay by comparing the results with different approximations. The estimated partial widths are all safely under the upper limits of the experimental data. Moreover, we find the branching ratio of D_{s1}(2536) rightarrow D_s^*gamma /D_s gamma are large enough to be detected, which could be searched by further experiments in Belle II and LHCb.
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