The galaxy presents an elliptical morphology, appearing largely smooth and featureless. Its shape is somewhat elongated, though not highly so. The core exhibits a yellowish hue, suggesting an older stellar population. Moving outwards from the center, the color gradually shifts towards a bluish tint, potentially indicating the presence of younger stars in the outer regions, although the distinction is subtle. There is no clear evidence of spiral arms or a well-defined disk structure. The galaxy appears relatively undisturbed, lacking any significant signs of ongoing mergers or major tidal disruptions. A slight asymmetry in the outer regions might hint at minor gravitational interactions, but further investigation is needed to confirm this.
