The galaxy presents as a spiral type, exhibiting distinct, well-defined spiral arms. The winding of the spiral arms appears relatively tight. These spiral arms show a dominant two-arm structure, although a definitive count is somewhat challenging. The central bulge is moderately sized and appears to be a prominent feature. The disk is viewed face-on. There is no sign of strong bar structure. No major merger is apparent, but some minor disturbances can not be ruled out.
