The galaxy presents as a well-defined spiral structure, exhibiting tightly wound spiral arms. The central bulge appears prominent and moderately sized, suggesting a classification along the lines of an early-type spiral. While the bulge displays a yellowish-white color, indicating an older stellar population, the spiral arms exhibit patches of bluer hues.

The galaxy displays a slight inclination relative to our line of sight, with the disk predominantly facing us. No major signs of ongoing mergers or significant disturbances can be detected within this galaxy.
