[2] A patchy emission is found having a low-surface brightness of around 22 R magnitude arcsec−2 ,based on Hubble Space Telescope (HST) imaging on the host galaxy.

[4] In addition, IRAS 07598+6508 has several star clusters located both west and south, based on a HST optical image.

[10] It has a spectrum being influenced by its tapered broad line region with a full width at half maximum measurement of 1780 km s−1.

This presence of clumps indicates the emission originates from OB associations and is the key to signs of recent star formation in the galaxy.

[12] A NICMOS image of IRAS 07598+6508, finds electromagnetic radiation is controlled by a source of light from the nucleus although low-level emission is also visible right up to ~ 2" radius.