The galaxy presents a face-on spiral morphology, exhibiting well-defined spiral arms. These arms are tightly wound, emanating from a central bulge. The bulge appears moderately prominent. The spiral arms show evidence of active star formation, indicated by the presence of knotty regions. There is a suggestion of a bar-like structure within the central region, although it isn't prominently defined. The galaxy disk is quite large, but is also fairly thin. The overall structure of the galaxy appears relatively undisturbed, lacking significant signs of recent major merger activity.
