IC 4329A, also commonly referred as PGC 49051 is a Seyfert galaxy in the constellation of Centaurus.

The declination of IC 4329A is approximately -30.2 degrees and was first discovered by Wilson A. S. & Penston, M. V. in 1979.

[1] This galaxy was first described by using an X-ray spectro-polarimetric analysis as an extremely bright Seyfert galaxy on account of the width of H-alpha (13,000 km/sec) and the high H-beta luminosity.

[7] Additionally, dust components in IC 4329A have been detected mainly in the interstellar medium of its host galaxy as well as its nuclear component located in the active torus.

[8] The supermassive black hole in IC 4329A is estimated to be 6.8+1.2−1.1 x 107 Mʘ.