This galaxy exhibits a prominent disk structure with clear evidence of spiral arms. The spiral arms appear somewhat fragmented and display a moderately wound morphology. A central bulge is present, though it does not appear to be the dominant feature of the galaxy. There appears to be a slight bar structure. Evident distortions within the spiral arms may indicate ongoing interactions or minor mergers. The galaxy's overall light distribution is concentrated toward the center with distinct spiral arms extending outward. Some regions appear brighter or more active in terms of star formation.
