The galaxy presents as a spiral type, exhibiting a prominent disk structure. The spiral arms are distinct and widespread across the galaxy, suggesting a well-defined morphology. The winding of the spiral arms appears intermediate, not tightly wound nor extremely loose. Two major arms are visible in the image. A central bulge is clearly present, it constitutes a significant fraction of the galaxy's visible light, indicating a substantial stellar population concentrated at the galaxy's core. The galaxy's disk is not oriented edge-on, affording a face-on view that allows detailed examination of the spiral structure. No indications of major ongoing mergers are immediately apparent, though minor irregularities or disturbances cannot be entirely ruled out. The image resolution allows for the classification of a barred structure, or lack thereof, within the central region.
