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We present BVRI photometry of supernova 2011fe in M101 from 2.9 to 182 daysafter the explosion. The light curves and color evolution show that SN 2011febelongs to the "normal" subset of type Ia supernovae, with $\Delta m_{15}(B) =1.21 \pm 0.03$ mag. After correcting for extinction and adopting a distancemodulus of $(m - M) = 29.10$ mag to M101, we derive absolute magnitudes $M_B =-19.21$, $M_V = -19.19$, $M_R = -19.18$ and $M_I = -18.94$. We compare visualmeasurements of this event to our CCD photometry and find evidence for asystematic difference based on color.

BVRI Photometry of SN 2011fe in M101