The galaxy presents as a disk-shaped structure with a noticeable central bulge. The bulge exhibits a yellowish hue, potentially indicative of an older stellar population. Moving outward from the bulge, the disk appears relatively smooth and somewhat elongated, showing a subtle gradient in color. The disk transitions into a more bluish tint, possibly due to the presence of younger, hotter stars. There appears to be a slight asymmetry in the shape of the galaxy, where one side of the disk seems more extended than the other. The lack of clearly defined spiral arms and the overall smoothness suggest this could be an early-type spiral galaxy.
