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In the context of holography, the Einstein ring of an AdS black hole (BH) inmassive gravity (MG) is depicted. An oscillating Gaussian source on one side ofthe AdS boundary propagates in bulk, and we impose a response function toexplain it. Using a wave optics imaging system, we obtain the opticalappearance of the Einstein ring. Our research reveals that the ring can changeinto a luminosity-deformed ring or light spots depending on the variation ofparameters and observational positions. When observers are positioned at thenorth pole, the holographic profiles always appear as a ring with concentricstripe surroundings, and a bright ring appears at the location of the photonsphere of the BH. These findings are consistent with the radius of the photonsphere of the BH, which is calculated in geometrical optics. Our studycontributes to a better understanding of the analytical studies of holographictheory, which can be used to evaluate different types of BHs for a fixed wavesource and optical system.

Holographic Einstein Rings of an AdS Black Hole in Massive Gravity