The galaxy presents a defined disk structure. Spiral arms are clearly visible and exhibit a relatively distinct, two-armed morphology. These arms are moderately wound, displaying neither a tightly wrapped nor exceptionally loose configuration. A central bulge is present, appearing substantial in size, but not entirely dominant relative to the disk. Evidence suggests a barred spiral structure, with a moderately prominent bar feature extending across the central region. There are no immediately apparent signs of a major merger event. The general appearance is suggestive of a well-formed spiral galaxy.
