The galaxy presents a notable spiral structure. The arms appear somewhat flocculent and display varying degrees of winding, trending toward a moderately-wound configuration. The central bulge exhibits a yellowish hue, potentially indicative of an older stellar population. The arms show a bluer tint, suggesting ongoing star formation regions within the disk. Overall, the galaxy appears to be an actively star-forming spiral galaxy, displaying a dynamic disk morphology. There is a potential presence of a smaller structure or tidal debris indicating a past minor merger event.
