NGC 3430 is classified as a well-known example of an SAc spiral galaxy with no central bar structure but has spiral arms found open and clear-defined.[2] Moreover, it is also a Wolf-Rayet galaxy, with star-forming regions[3] and forms a pair with NGC 3424, a nearby starburst galaxy.[4] According to a 1997 study presented by researchers, these galaxies are clearly showing signs of tidal interaction.[5]
Two supernovae have been observed in NGC3936: SN2004ez (typeII, mag.17.3),[6][7] and PSNJ10520833+3256394 (typeIIb, mag.17.8).[8]