The galaxy presents as a spiral type, with a clearly defined disk structure. Approximately 3/4 of the galaxy is visible. The spiral arms appear prominent and somewhat flocculent, with a range of winding tightness observed. Some arms wind more tightly around the central bulge.

There is a moderate-sized bulge in the center that is neither extremely dominant nor negligible. The bulge region exhibits a yellowish hue, suggesting an older stellar population.

Evidence for a bar structure is present, although not overwhelmingly dominant.

There is a hint of a slight distortion in the overall morphology, possibly indicating a minor interaction or disturbance. Additionally, there are regions of apparent active star formation within the spiral arms, evidenced by bluish concentrations of light.
