The galaxy appears to be a spiral galaxy, observed at a high inclination angle, possibly edge-on. A prominent central bulge is visible, exhibiting a yellowish hue. The disk component is also evident, though partially obscured by dust. The disk displays a bluish tint, suggesting ongoing star formation activity. There are indications of disturbances within the disk structure, with some asymmetries noted. The galaxy's overall structure suggests a system with signs of recent or ongoing interactions or internal dynamic processes.
