NGC 4459 has a central flocculent dust disk that surrounds an inner ring.[6][7] Also, there appears to be evidence of ongoing star formation in the disk .[7]
^Young, Lisa M.; Bureau, Martin; Cappellari, Michele (23 December 2007). "Structure and Kinematics of Molecular Disks in Fast‐Rotator Early‐Type Galaxies". The Astrophysical Journal. 676: 317–334. arXiv:0712.4189. doi:10.1086/529019. S2CID119215566.