We report the photometric observations of an SU UMa-type dwarf nova VW CrB during two superoutbursts in 2001 and 2003 and a normal outburst in 2003 .
Superhumps with a period of 0.07287 ( 1 ) d were observed during the 2003 superoutburst .
The change rate of the superhump period was positive .
During the normal outburst , there are some hint of modulation up to a 0.2-mag amplitude .
However , any periodicity was not found .
The recurrence cycles of the normal outburst and the superoutburst , and the distance were estimated to be \geq 50 d , 270 \sim 500 d , and 690 ^ { +230 } _ { -170 } pc , respectively .
These recurrence cycles are usual values for an SU UMa-type dwarf nova having this superhump period .
The superhump period of VW CrB was the longest among those of the SU UMa stars with positive derivatives of the superhump period .
The coverage of our observations was , however , not enough , and the variation of the P _ { SH } change rate of VW CrB is still unknown .
A superhump regrowth and a brightening were seen near the end of the plateau phase .
Measuring the deviation of the start timings of the brightening and the superhump regrowth ( > 2 days in VW CrB ) will be a key to reveal the mechanism of these phenomena .