The galaxy presents as an elliptical morphology, appearing largely smooth and featureless. The light profile suggests a centrally concentrated spheroid with a gradual decrease in surface brightness moving outwards. The core region exhibits a yellowish-white hue, indicative of an older stellar population. There is a slight bluing visible in the very center, suggesting ongoing star formation. The galaxy appears relatively isolated, with no immediately obvious signs of tidal interactions or significant morphological disturbances. The overall structure indicates a system dominated by random stellar motions with limited dust and gas content in its outer regions.
