This galaxy presents a spiral morphology. Distinct spiral arms are observed emanating from the central bulge. The arms appear somewhat tightly wound in some sections and more open in others, and at least two primary arms are visible. The central bulge appears moderately sized and exhibits a yellowish hue, suggesting an older stellar population. The spiral arms show a bluer tint, which indicates a younger stellar population and ongoing star formation. There are potential signs of minor tidal disturbances or interactions, as evidenced by slight asymmetries or faint extensions in the outer regions. The main body of the galaxy does not appear to be edge-on.
