The galaxy presents a spiral morphology, with a moderately sized bulge that shows a yellow-ish color that might indicate an older stellar population. The disk component is visible and displays evident spiral arms. These arms appear fairly well-defined, tracing a mostly complete spiral structure. The spiral arms are quite flocculent but exhibit a median winding pattern. A bar is also visible crossing the central part of the galaxy. The inclination is significant but still face-on, allowing us to see a good portion of the galaxy.
