The boxy bulge of NGC 3573 (Fig. 8) is at low surface brightness levels
very asymmetric. On one side of the minor axis the bulge clearly ends
and a perturbed warped disk component follows, but on the other side
bulge and disk component are merged and largely spread into a diffuse
structure which is also asymmetric with respect to the major axis.
Overexposed center, strong dust lane, very faint dist arms. IBm V 12'
=ESO 377- G 22