II, which has $0\farcs26$ pixels and a 05 field-of-view. We imaged through the Johnson-Cousins [*UBVRI*]{} filters on the nights of 1–3 June 2000. These 38$\times$38 dithered fields are shown in Figure \[figure:gcfields\]. The center field (CTR) is centered on the galaxy. The northeast (NE) field was chosen to follow the faint halo light out along the major axis, while the south (S) field was chosen to avoid galactic cirrus and observe a large “sky” area, as determined from Malin’s deep photographic image (Malin 1978). The [*V*]{}-band image of each field is shown in Figures \[figure:GCctrV\], \[figure:GCneV\], and \[figure:GCsV\]. The total exposure times in [*UBVRI*]{} were 3600s, 1500s, 1800s, 1000s, and 1000s, respectively, for the CTR field. For the other two fields, we went slightly deeper in [*U*]{},[*R*]{}, and [*I*]{} with exposure times of 3900s, 1500s, 1800s, 1800s, and 1500s, respectively. We split our observations in each band into a series of five dithered exposures (six for [*U*]{} and [*I*]{} in the NE and S fields). Conditions were non-photometric on the first night, but were photometric for the remainder of the observing run. All images taken on the first night were calibrated by images taken on the subsequent nights. The seeing 