The galaxy presents as a spiral type, viewed at a significant angle relative to face-on. Two spiral arms appear to originate close to the galactic center and are wound relatively tightly. The central bulge is moderately prominent and exhibits a yellowish hue, suggesting an older stellar population. Faint blue regions are observed in the arms, indicating regions of recent star formation. The disk component is not perfectly smooth; it exhibits a slight clumpy texture, which might be the result of minor gravitational interactions or internal processes. There is no visible bar. The galaxy is not undergoing a major merger, but there is a slight hint of minor disturbance in the disk morphology.
