The galaxy presents a primarily face-on orientation relative to the observer's line of sight. A notable feature is the distinct, albeit somewhat diffuse, spiral arm structure extending outwards from a central bulge. The spiral arms exhibit a bluer hue, suggesting regions of ongoing star formation activity. The central bulge appears more yellowish-white, indicative of an older stellar population. There's a moderate bulge, which appears smooth. The arms appear fairly symmetric. Based on its structure, the galaxy can be classified as a spiral galaxy. There are no signs of a major merger occurring with another galaxy. The galaxy has a slight tilt and is largely disk-shaped. There are no clear signs of a bar structure. 
