The galaxy presents as a centrally concentrated, elliptical-like structure. The core exhibits a bright, yellowish-white hue, suggesting a population of older stars. The light smoothly transitions outward, diminishing in intensity without displaying prominent spiral arms or distinct features. There's a subtle flattening suggesting it may be not perfectly spherical. No signs of tidal disturbances, major mergers, or intense star-forming regions are readily apparent. The overall smooth morphology is consistent with an evolved system where the star formation rate is relatively low. The galaxy appears to be fairly massive and quiescent, suggesting a considerable stellar population.