[7] When observed in radio waves the galaxy is asymmetric, with emission being from the nucleus, three star-forming regions and a ridge towards NGC 2444.

[3] Observations of carbon monoxide emission indicate that NGC 2445 still has abundant gas and star formation rates will increase.

[9] Hubble Space Telescope has uncovered dark filaments of gas in the starburst galaxy's bright core.

[3] When observed in radio waves the core isn't very compact and its spectrum indicates the presence of a starburst region with an age between 1.5 and 5 million years.

A filament of this shells points towards the galaxies indicating that it is a superbubble associated with them[10] or a tidal tail.