We report new detailed surface U,B,V,R, and I photometry of 81 stellar structures in the disk of the barred galaxy NGC 3367 .
The images show many different structures indicating that star formation is going on in the most part of the disk .
NGC 3367 is known to have a very high concentration of molecular gas distribution in the central regions of the galaxy and bipolar synchrotron emission from the nucleus with two lobes ( at 6 kpc ) forming a triple structure similar to a radio galaxy .
We have determined the U,B,V,R, and I magnitudes and U - B~ { } ,B - V~ { } ,U - V~ { } , and V - I colors for the central region ( nucleus ) , a region which includes supernovae 2003 AA , and 79 star associations throughout NGC 3367 .
Estimation of ages of star associations is very difficult due to several factors , among them : filling factor , metallicity , spatial distribution of each structure and the fact that we estimated the magnitudes with a circular aperture of 16 pixels in diameter , equivalent to 6 ^ { \prime \prime } .8 \sim 1.4 kpc .
However , if the colors derived for NGC 3367 were similar to the colors expected of star clusters with theoretical evolutionary star tracks developed for the LMC and had a similar metallicity , NGC 3367 show 51 % of the observed structures with age type SWB I ( few tens of Myrs ) , with seven sources outside the bright surface brightness visible disk of NGC 3367 .