The galaxy presents a generally smooth, elliptical morphology. The central region exhibits a concentrated, bright, yellowish-white core, suggesting a higher density of older stellar populations. Progressing outwards from the core, a subtle transition to a bluish halo is observed. This halo appears mostly smooth and regular, showing no prominent spiral arm structures or distinct features. There are subtle indications of minor disturbances. The shape appears closer to round rather than elongated, and the overall structure implies a relatively evolved system.
