The galaxy exhibits a well-defined spiral structure. Two prominent spiral arms emanate from the central bulge region and extend outwards. These arms are moderately wound, displaying a noticeable pitch angle relative to the galaxy's center. The arms appear to be fairly continuous, showing no significant breaks or bifurcations along their length.

The central bulge appears relatively small and subdued in size. There's a strong bar feature bisecting the central bulge, oriented approximately horizontally in this image.

The disk component shows some visible dust lanes. These lanes are mostly concentrated within the spiral arms. There's some evidence of ongoing star formation throughout the disk, as indicated by some localized bright areas within the spiral arms.

The galaxy displays an overall blueish-white color. The spiral arms are bluer in coloration, likely due to active star formation. The central bulge appears yellower. The galaxy appears to be relatively undisturbed, displaying no strong signs of interaction or recent merger events.
