The galaxy presents an elliptical morphology, appearing largely smooth and relatively featureless. The core exhibits a concentrated, bright, yellowish-white luminosity, suggesting an older stellar population. A diffuse, somewhat fainter halo extends outward from the core. The halo shows hints of a slight blue tinge, possibly indicating some presence of younger, hotter stars, albeit in a smaller proportion compared to the core. The galaxy does not appear to be undergoing any major merging events or significant tidal disturbances. Its overall structure suggests a system that has largely completed the process of hierarchical assembly and is now evolving passively.
