The galaxy presents as a slightly inclined disk galaxy. There appears to be a central bulge region that is slightly brighter and more concentrated than the surrounding disk. A spiral structure seems to be present. It is moderate to weak, with arms that are somewhat flocculent in appearance. The galaxy exhibits a blue hue, suggesting the presence of ongoing star formation. No obvious signs of major interactions or mergers are apparent, and it appears that the galaxy is relatively undisturbed.
