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We present photometric observations of transit of the exoplanet HAT-P-24busing the Rozhen 2 m telescope. Its solution gives relative stellar radiusr_{s}=0.1304 (a/R_{s}=7.669), relative planet radius r_{p}=0.01304 and orbitalinclination of 90 degree. The calculated planet radius is R_{p}=1.316 R_{J} andcorresponds to planet density of rho_{p}=0.37 g cm^{-3}. Our parameter valuesare between those of the previous two solutions. We did not find evidences ofTTV and TDV signals of HAT-P-24b.

Solution of newly observed transit of the exoplanet HAT-P-24b: no TTV and TDV signals