The galaxy appears to be a spiral galaxy viewed at a moderate inclination. It has a prominent central bulge, which exhibits a yellowish-white hue, suggesting an older stellar population. The disk is visible, showing a hint of spiral structure with a bluish tint, indicative of ongoing star formation. The arms are not clearly defined but are present. There is some dust obscuration throughout the disk but the dustlanes are not particularly pronounced. No strong signs of recent major merger activity are apparent; the galaxy appears relatively undisturbed, though there may be minor disturbances to the disk. Overall, the galaxy exhibits characteristics consistent with a spiral galaxy with a mix of old and young stellar populations.
