Much of this meeting has focused on possible ways in which nuclear mass concentrations - such as steep central cusps or black holes - influence the global structure of elliptical galaxies. This discussion is motivated by the apparent dichotomy (Kormendy, these proceedings) between faint ellipticals (which have steep central profiles, ``disky'' isophotes, and rapid rotation) and bright ellipticals (which have shallow central profiles, ``boxy'' isophotes, and slow rotation). But other factors besides central density profile can influence galaxy structure.