The galaxy presents as a spiral, with a prominent central bulge that appears relatively bright and concentrated. The spiral arms are well-defined and extend outwards from the central region. A strong bar-like structure appears to bisect the central bulge. The arms show a winding pattern that tends towards tight, with some segments displaying medium winding. Star formation regions are visibly scattered throughout the arms, identifiable by their bluer hue. Dust lanes are also apparent within the spiral arms. The overall impression is of a well-formed spiral structure. 
