The galaxy presents as a grand design spiral, with two prominent spiral arms emanating from a central bulge. The spiral arms appear loosely wound and extend considerably from the galactic center, indicating a relatively low shear rate.

The central bulge exhibits a moderate size relative to the overall galactic disk. Its color is subtly more yellow, suggesting an older stellar population compared to the disk.

Star formation appears to be active within the spiral arms. A bluish hue is observed along the arms, indicative of the presence of young, hot, massive stars. There are also areas of reddish emission along the spiral arms, that could indicate areas of dust and gas.

There is no visible bar structure. There are no significant signs of a major ongoing merger, although there might be minor disturbances visible in one of the spiral arms. The galaxy is viewed close to face-on.
