  Modified Newtonian Dynamics (MOND) and its relativistic version - TeVeS offer
us an alternative perspective to understand the universe without the demand of
the elusive cold dark matter. This MONDian paradigm is not only competitive
with the conventional CDM in a large range of scales, but also even more
successful in the galactic scale. Recently, by studying 6 lensing systems,
Ferreras et al. (2008) claimed that MOND still needs dark matter even in
galactic scales. When we study the same systems, however, we yield an opposite
conclusion. In this contribution, we report our result and conclude that MOND
does not need dark matter in galactic lensing systems. Furthermore, we extend
our study to 22 SLACS (Sloan Lens ACS Survey) lenses, and obtain the same
conclusion as well, i.e., no dark matter is needed in elliptical galaxies.
