The second IC lists a corrected position (per Delisle Stewart) of RA 03 25 44, NPD 124 06, and adds "annular; h's place was very rough"
Based on recessional velocity measurements of 1440 and 1905 km/sec (!), NGC 1350 is 65 to 90 million light years away, in good agreement with equally variable redshift-independent distance estimates of 55 to 85 million light years. Given that and an apparent size of 6 by 3 arcmin, it is between 115 and 145 thousand light years in diameter.

A member of the Fornax Cluster, the second richest cluster of galaxies within 100 million light years, and a Seyfert galaxy (type Sy 1.8). Based on recessional velocity of 1635 km/sec, about 75 million light years away, in good agreement with redshift-independent distance estimates of 35 to 80 million light years, and the estimated distance of the cluster, of about 60 million light years. Given that and apparent size of 11.2 by 6.2 arcmin, about 200 thousand light years across. A rotating density wave triggers the formation of new star clusters in the spiral arms, helps maintain the structure of the bar, and funnels material into the bar, feeding its growth and most likely, that of a supermassive black hole hidden within the dusty clouds which partially obscure the bar. Because of the huge mass of the galaxy (more than a trillion solar masses), the bar rotates at well over a thousand miles a second, but even at such speeds the spiral arms take three or four hundred million years to move once around the galaxy's vast circumference.