The galaxy appears to be a spiral galaxy exhibiting a defined disk structure. Prominent spiral arms are visible, suggesting active star formation regions throughout the disk, evidenced by bluish hues. The arms appear tightly wound around the central bulge. A moderate sized bulge is present, appearing yellowish-white, indicating an older stellar population. There is no obvious presence of a strong bar feature. The morphology does not strongly indicate any signs of major merging activity or significant disturbance. The overall structure suggests a well-formed spiral galaxy with ongoing star formation within its spiral arms.
