Intensity profiles of NGC 2276 as a function of galactocentric radius. Top: F555W image divided into eight sectors with constant azimuthal separations of 45°. The concentric ellipses show regions with constant galactocentric distance of 3, 6, 9, and 12 kpc. White dotted line represents 3-σ background noise level contour. Bottom: Surface brightness radial profile in the F555W band for each of the 8 sectors in bin size of 0.5 kpc. Three dotted lines represent 1, 2, and 3-σ background noise level. All data points have a S/N above 5.