The galaxy presents a distinct spiral morphology.  While not perfectly face-on, its disk-like structure is clearly visible, with spiral arms emanating from a central bulge. The bulge appears moderately sized relative to the overall disk. The arms exhibit a tightly wound structure, suggesting a relatively high shear rate within the disk. The color profile of the galaxy shows a concentration of blue light, particularly within the spiral arms. This is indicative of ongoing star formation within these regions. The overall shape displays ellipticity, with the major axis oriented at an angle. Some minor asymmetries or disturbances in the outer regions of the disk suggest potential interactions or past mergers.  No prominent bar structure is apparent.
