The galaxy exhibits a spiral morphology, with a central bulge region that appears moderately prominent. Faint spiral arms emanate from the central region. The arms appear to be winding from medium to tight around the bulge region. There is no evidence of a bar structure present in the galaxy. The arms show noticeable blue color, suggesting ongoing star formation within the galaxy. The outer regions of the galaxy disk appear relatively smooth and undisturbed. Based on the distribution of light and the relatively concentrated central region, the galaxy likely has a Sersic index between 1 and 2.
