The galaxy presents as a spiral galaxy with a relatively bright, concentrated central bulge region exhibiting a yellowish hue, suggestive of an older stellar population. Extending from the central bulge are two prominent spiral arms. These arms are somewhat tightly wound and present a bluish tint indicative of ongoing star formation. The disk appears relatively undisturbed, showing no obvious signs of a major ongoing merger event. Faint structure exists at the edge of the arms, suggesting weak disturbance. There appears to be a weak bar-like structure present. Overall, the morphology suggests a galaxy that is actively forming stars within its spiral arms while hosting an older stellar population in its bulge.
