The observed galaxy presents as a spiral galaxy, exhibiting a disk-like structure. Prominent spiral arm features are visible, appearing somewhat tightly wound. There is an apparent central bulge that appears moderately sized. The galaxy is observed at an angle, not quite edge-on, but not fully face-on either, thus the spiral structure is somewhat obscured.

The galaxy displays a color gradient; the central bulge region appears more yellow/white, indicating an older stellar population. The spiral arms show a slightly bluer hue, consistent with the presence of younger, hotter stars.

There are no obvious signs of a major ongoing merger, though minor disturbances or interactions cannot be ruled out based on the presented image. There may be a weak bar-like structure extending from the central bulge, but this is not definitive. Overall, the galaxy presents as a relatively undisturbed spiral system.
