The observed galaxy presents an elliptical morphology, exhibiting a relatively smooth light distribution without readily discernible spiral arms or prominent features. Its shape deviates slightly from a perfect circle, displaying a moderate elongation. The galaxy's core appears bright and concentrated, with a gradual decrease in luminosity towards its outer regions. The color profile indicates a dominance of older stellar populations, manifested by the yellowish-red hue, potentially suggesting a relatively quiescent star formation history. No major signs of tidal disturbances, ongoing mergers, or significant starburst activity are apparent. The galaxy appears relatively isolated, showing no immediately interacting companions within its vicinity.
