We have investigated the morphology and physical properties of spiral galaxies use the SDSS DR7. The redshift of our sample galaxies less than 0.01. We found 1013 spiral galaxies from 7110 galaxies with z less than 0.01 and determined the Hubble types of these spiral galaxies by visual inspection and analyzed their physical properties. For 543 galaxies we classified their bar type (SA, SAB, SB) but bar types were not determined for 470 galaxies due to high inclinations. The luminosities and colors of spiral of early type spiral galaxies are brighter and redder than the late type spiral galaxies. The central concentration of luminosity decreases from the erly type galaxies to the late types. The intermediate type spiral galaxies show the largest size while the late type spiral galaxies have the smallest size. From the analysis of the emission lines from the nuclear regions of galaxies, we found that the 232 spiral galaxies have AGNs. We found 72 candidates of the dwarf spiral galaxies which are smaller than 3kpc and fainter than Mr=-17.