a) WHIRC H band image from the WIYN 3.5-m telescope, shown in a log scale. WIYN’s 0.8′′ resolution allows us to examine the internal structure of the nucleated bulge, offering a level of detail unavailable in IRAC images. b) The same image with added contours that detail the internal structure of the nucleated bulge. This image also features the brightness minimum in the lower left-hand corner, clearly denoting the offset between the two extrema. Both parts are rotated counter-clockwise 135° as compared to Fig. 2a.