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Spiral Galaxy NGC 1512. NGC 1512 is a barred spiral galaxy approximately 38 million light-years away from Earth[2] in the constellation Horologium. Image Credit: NASA, ESA, Hubble Space Telescope
NGC1512/10, SINGG Survey
This image shows a strong interaction between the barred spiral NGC1512 and its Blue Compact Dwarf (BCD) companion, NGC1510. Star formation in NGC1512 is concentrated into two rings; the inner one has the strength of a starburst. Surprisingly star formation is even stronger in the BCD NGC1510, which can be seen to the lower right of NGC1512. This pair ilustrate how galaxy interactions are able to trigger starbursts.
credit line: The SINGG Survey Team and NOAO/AURA/NSF
NOAO
NGC 1512 Nucleus by Judy Schmidt Via Flickr: The center of NGC 1512 with some rather heavy processing to bring out the faint inner dust spiral. LEGUS: Legacy ExtraGalactic UV Survey Red: hst_13364_69_wfc3_uvis_f814w_sci Green: hst_13364_69_wfc3_uvis_f555w_sci Blue: hst_13364_69_wfc3_uvis_f438w_sci, hst_13364_69_wfc3_uvis_f336w_sci, hst_13364_69_wfc3_uvis_f275w_sci North is up.

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NGC 1512 (Spiral Galaxy) (C) NASA
http://www.gingadan.com/ngc1512.html