The black hole shadow is fundamentally connected to the structure of light rings and the photon region in the background geometry. We investigate the photon region boundary in a generic asymptotically flat, stationary, axisymmetric black hole spacetime that admits spherical photon orbits (SPOs). Explicit expressions possessing real solutions are provided for the photon regions boundary purely in terms of the background metric functions, independent of the photons parameters like energy or angular momentum, which are applicable to both separable and nonseparable spacetimes. We further analyze its common features, including overlap with the ergoregion and rotation sense of SPOs. Additionally, light rings are identified at the extrema of the photon region boundary curves in the $(r,\theta )$ plane. Our approach is validated against a few exact black hole solutions. Implications are discussed.

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• Alternative gravity theories
• Classical black holes
• General relativity
• General relativity equations & solutions
• Gravitation