Top: color image of SB(lens)0 galaxy NGC 4452 from the SDSS g,r,i images via http://www.wikisky.org. The bulge—which proves to be pseudo—is so tiny that it is almost invisible. The inner disk is edge-on and very flat; it again consists of two shelves in surface brightness. Including the outer, thicker disk, these three shelves are signatures of a bar, lens, and disk. Bottom: ellipticity and surface brightness μ _V along the major axis of NGC 4452 measured by fitting ellipses to the isophotes in the ACS and SDSS g-band images. The five dashed curves show a decomposition of the profile inside the fit range (vertical dashes). The nucleus, bulge, bar, lens, and disk are represented by Sérsic functions with indices n as given in the figure. The sum of the components (solid curve) fits the data with an rms of 0.044 V mag arcsec ⁻².