The galaxy presents an elliptical morphology, appearing largely smooth and featureless. The central bulge exhibits a concentrated luminosity, transitioning gradually into a fainter, more diffuse halo. The overall color profile suggests a dominance of older stellar populations, with a redder hue concentrated in the central regions. There is a subtle indication of a disk-like structure, though it is not sharply defined. No prominent spiral arms or significant dust lanes are discernible. The galaxy appears relatively undisturbed, without any obvious signs of recent major mergers or tidal interactions. The absence of strong blue colors indicates low ongoing star formation activity.
