The galaxy presents as a spiral type, with a disk-dominated structure. The spiral arms are prominent, displaying a loosely wound morphology. Two distinct arms are readily apparent. There is an indication of a central bulge, although it does not appear overly significant in size. Color gradients suggest some level of ongoing star formation, particularly within the spiral arms. There is no readily apparent bar structure. The galaxy exhibits no signs of major interactions or mergers, although a subtle disturbance cannot be entirely ruled out. The disk is oriented at a relatively low inclination with respect to the observer's line of sight, as its edge is not apparent.
