The Large Binocular Camera (LBC) is a double wide-field imager for the 
Large Binocular Telescope. It is designed for seeing-limited observations 
in the wavelength range from the near UV to 1 micron, over a 1/2 degree 
diameter field of view. After describing the instrument, I will report on 
the current status of the project. At the moment of this writing (February 2005), 
the Red Channel of LBC is going to be integrated in the laboratory, while the 
Blue Channel has already been installed at the telescope and most of the 
commissioning operations have been completed, in parallel with the telescope 
commissioning. The first light of LBT with LBC Blue is foreseen in late 
spring - early summer 2005.