The galaxy presents a generally elliptical morphology. The central region exhibits a high concentration of light, appearing smooth and yellowish-orange in color, indicative of an older stellar population. The luminosity gradually decreases outwards, transitioning into a fainter, diffuse halo. There are no prominent spiral arms or dust lanes visible. The overall appearance suggests a relatively undisturbed system, with no obvious signs of ongoing major merger activity. The color gradient indicates a lack of significant recent star formation, as the bluer regions associated with younger, hotter stars are absent. Some minor irregularities might be present in the outer regions, hinting at possible minor interactions or internal disturbances. The shape is neither perfectly round nor highly elongated, leaning towards an intermediate classification.
