The galaxy presents a distinct spiral morphology. Two tightly wound spiral arms emanate from a central bulge, appearing somewhat small relative to the overall disk size. The arms exhibit a blueish hue, potentially indicative of ongoing star formation activity. The bulge appears yellow-white, suggesting an older stellar population. The galaxy does not show any obvious signs of major interaction or merging with other galaxies, though some minor distortions might be present in the outer arms. The galaxy is face-on, allowing for a clear view of its spiral structure.
