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We report on MASTER optical observations of an afterglow-like optical and X-ray transient AT2021lfa/ZTF21aayokph. We detected the initial steady brightening of the transient at 7σ confidence level. This allowed us to use smooth optical self-similar emission of GRBs model to constrain the explo-sion time to better than 14 minutes as well as to estimate its initial Lorentz factor Γ0=20±10. Taking into consideration the low Γ0 and non-detection in gamma-rays, we classify this transient as the first failed GRB afterglow. Key words: stars: gamma-ray burst: general, transients: gamma- https://www.youtube.com/watch?v=sh6t4VOhiHk&list=PLPW1HYb0Hl0qucM2cqLkzOKD9nTu1aznr&index=5 http://master.sai.msu.ru/ru/master2022/program