[9] The core component is suggested to be significantly variable, hinting at the presence of jet activity in RX J1633.3+4718.

[9][4] The north component on the other hand, is fainter and located at a position angle of 352°, away from the core by 3.8 arcsec.

[11] The accretion disk of RX J1633.3+4718 is shown to have ultrasoft excess X-ray emission.

It is lower than 0.5 KeV with the temperature of the galaxy's disk estimated to be 40 electronvolts based on a disc model for soft excess.

The mass of the black hole in RX J1633+4718 is estimated to be 3 x 106 Mʘ[8] while a bolometric luminosity of Lbol ≈ 1.51 x 1044 erg s−1 was derived from an unabsorbed flux measurement in a 0.001-100 KeV energy band.