The
morphological classification of this galaxy is (R)SAB(s)a,[7] which indicates a spiral galaxy with a weak-bar around the nucleus (SAB), no ring around the bar (s), an outer ring (R), and tightly-wound
spiral arms (a). It is inclined by an angle of 57° to the
line of sight from the
Earth, with the long axis oriented at a
position angle of 324°.[5] The disk of gas and stars shows a noticeable warp, and there is a pronounced asymmetry in the distribution of neutral hydrogen and
H II regions.[11]
The core region contains a suspected weak
active galactic nucleus plus a circumnuclear ring containing
star clusters and
supernova remnants at a distance of ~280 pc from the center. These form a ring of peculiar "hot spots".[12] It was formerly identified as a possible
Seyfert galaxy,[5] but evidence now points to
starburst activity in a ~500 pc radius around the center.[13] A probable outflow of gas is directed to the north-east from the nucleus, forming prominent dust lanes.[5] The high level of
star formation in this galaxy and the nearby
NGC 1792 may indicate a recent, distant
tidal interaction between the two.[11]
The
type Ia supernovaSN 1993af was discovered in November 1993 at 220″ east and 94″ north of the galactic nucleus.[14][15]
^
abSinnott, Roger W.; Perryman, Michael A. C. (1997). Millennium Star Atlas. Vol. 1. Sky Publishing Corporation and the European Space Agency.
ISBN0-933346-84-0.