The galaxy presents as a relatively compact object with a flattened, elliptical morphology. The central region exhibits a high degree of luminosity, appearing nearly spherical and a yellow-white hue, suggesting a high concentration of older stellar populations. This bright central bulge fades outward into a more diffuse halo. The outer regions of the galaxy show a bluer tint, hinting at the presence of some younger stars and possibly ongoing, albeit subdued, star formation in the disk. There is a subtle hint of some minor disturbances in the disk.
