The galaxy presents a spiral morphology, with a central bulge that appears moderately prominent. The spiral arms are well-defined but relatively tightly wound, displaying a bluish hue suggestive of ongoing star formation. Dust lanes are present, contributing to the mottled appearance of the disk. The orientation of the galaxy is nearly edge-on, giving it an elongated shape. The overall structure indicates a galaxy that is actively forming stars within its spiral arms. The galaxy does not show evidence of a strong bar. The general color profile suggests an intermediate-mass system. There appears to be no merging or major disturbances occurring.
