The galaxy presents as a relatively well-defined spiral structure, viewed at a significant inclination. The central bulge appears prominent and exhibits a smooth, concentrated luminosity, likely indicative of an older stellar population. Surrounding the bulge, spiral arms are visible, displaying a tightly wound morphology. These arms appear somewhat flocculent in nature, with regions of enhanced star formation activity suggested by bluish tinges throughout the arms. Dust lanes appear to exist in parts of the galaxy. There are small bright spots distributed in the galaxy. The overall light distribution appears slightly asymmetrical, hinting at possible past interactions.
