NGC 4217 is an edge-on spiral galaxy which lies approximately 60 million light-years (18 million parsecs) away in the constellation of Canes Venatici. It is a possible companion galaxy to Messier 106 (NGC 4258). One supernova, SN 2022myz (type I, mag. 19), was discovered in NGC 4217 on 19 June 2022.
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References
Further reading Thompson, Thomas W. J.; Howk, J. Christopher; Savage, Blair D. (2004). "Hubble Space Telescope Imaging of Extraplanar Dust Structures in the Edge-On Spiral NGC 4217". The Astronomical Journal. 128 (2): 662–673. Bibcode:2004AJ....128..662T. doi:10.1086/422485.
External links Media related to NGC 4217 at Wikimedia Commons






