The galaxy presents as a spiral, viewed at an angle slightly off from face-on. The central bulge appears prominent and yellowish, suggesting a concentration of older stars. Faint spiral arms extend outwards from the bulge. The arms are not tightly wound, indicating a later-type spiral galaxy. There is evidence of ongoing star formation within the arms, which have regions of bluer light. One arm segment is very faint and undefined in comparison to the other. No strong bar structure is clearly visible. There might be some interaction or minor disturbance in progress, as there is a slight asymmetry in the morphology, particularly in the faintness of one of the arm structures. The galaxy displays a significant degree of central concentration and, likely, a supermassive black hole. 
