The galaxy presents as a spiral galaxy with a significant disk component. The spiral arms are well-defined and appear relatively tightly wound. There is a noticeable central bulge, but it is small compared to the overall size of the disk. The galaxy is nearly face-on, allowing for detailed observation of its spiral structure. The spiral arms exhibit a bluer hue, indicating the presence of younger, hotter stars. The galactic disk appears to be fairly smooth, with a moderate amount of patchy star formation evident in the spiral arms. A weak bar feature appears to run through the center of the galaxy. The galaxy appears undisturbed, showing no signs of major merging activity.
