1 INTRODUCTION  
2 DATA  
2.1 Sample of MaNGA AGN and AGN Narrow Line Region Maps  
2.2 WISE Mid-IR Colors  
2.3 Host Galaxy Morphology from SDSS Catalogs  
3 MORPHOLOGICAL MEASUREMENTS  
3.1 Identification of Bi-polar Ionization Cone  
3.2 Opening Angle of Ionization Cone  
3.3 Concentration  
4 RESULTS  
4.1 The Intrinsic Opening Angle of Ionization Cones  
4.2 Correlation Between NLR Morphology and Mid-IR Color of Dusty Torus  
4.3 Alignment Between Narrow-line Region and Host Galaxy  
5 DISCUSSION  
5.1 Tests of Unification Model – Type I / Type II Ratio  
5.2 Tests of Unification Model – Source of Obscuration  
6 CONCLUSION