The galaxy presents as a relatively smooth, disk-like structure viewed at an oblique angle. Its overall color is yellowish-white, indicative of an older stellar population. The central region is brighter and more concentrated, suggesting a significant bulge component. The outer regions exhibit a gradual decrease in luminosity, fading into the background. There is subtle evidence of a disk, but no distinct spiral arm structures are readily apparent. The axial ratio suggests it's not perfectly edge-on or face-on, but somewhere in between. There might be some minor disturbances or irregularities in the outer parts, but overall, the galaxy seems to have a fairly regular, well-defined shape.
