The galaxy presents a largely smooth morphology, appearing elliptical in shape. There is a dominance of light in the redder wavelengths, giving the galaxy a yellowish-red hue. This suggests an older stellar population is more dominant. The galaxy appears largely undisturbed, with no obvious signs of major mergers or tidal interactions. It shows a concentrated central bulge, with a gradual decrease in luminosity toward the outer edges. There is only a very weak presence of blue light, and no distinguishable disk.
