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Lorentz-Violating (LV) scenario gets involved through a bumblebee fieldvector field $B_\mu$. A spontaneous symmetry breaking allows the field toacquires a vacuum expectation value that generates LV into the system. AKerr-Sen-like solution has been found out starting from the generalized form ofa radiating stationery axially symmetric black-hole metric. We compute theeffective potential offered by the null geodesics in the bumblebee rotatingblack-hole spacetime. The shadow has been sketched for different variations ofthe parameters involved in the system. A careful investigation has been carriedout to study how the shadow gets affected when Lorentz violation enters intothe picture. The emission rate of radiation has also been studied and how itvaries with the LV parameter $\ell$ is studied scrupulously.

Bumblebee gravity with a Kerr-Sen-like solution and its Shadow