This galaxy presents as a spiral type, although the angle to the observer obscures a clear view of defined spiral arms. Hints of two spiral arms are visible. The arms appear loosely wound. There is no observed strong bar structure bisecting the galactic center, although a weak bar may be present. A bulge is visible, representing approximately moderate size relative to the galaxy's disk. There is no evidence of a major merger. Indications suggest the galaxy may be experiencing minor disturbances, with some asymmetries visible in the outer disk. Star formation is evident, although it is somewhat obscured by dust or distance.
