The galaxy appears to be a spiral galaxy viewed at an oblique angle, not quite edge-on. It exhibits a central bulge with a yellowish hue, suggesting an older stellar population. Fainter, bluer regions are observed in the disk, possibly indicating areas of more recent star formation. There are no apparent signs of a strong bar structure or a well-defined spiral arm structure. Some asymmetry is observed in the outer regions of the disk, suggesting possible minor gravitational interactions or disturbances. The overall smoothness of the light distribution points towards a well-mixed stellar population, but hints of possible disturbances exist.
