The galaxy presents as a spiral type, viewed at a relatively slight inclination from edge-on. Two distinct spiral arms are observable, originating from a central bulge. The spiral arms appear loosely wound. A bar structure may be present, although obscured by the bulge's luminosity. The central bulge appears moderately sized relative to the overall galactic disk. Star formation is evident along the spiral arms, indicated by the slightly bluer hue compared to the yellowish bulge. There is no obvious indication of major merging activity, although minor disturbances cannot be ruled out based on this image alone. The galactic disk dominates the visual profile.