The galaxy presents a largely smooth, elliptical morphology. Its color appears predominantly yellow-orange, suggesting a population of older stars. The central region exhibits a high degree of concentration. There is a subtle gradation in luminosity from the core outwards, with no distinct features such as spiral arms or a pronounced disk visible. The general roundness of the galaxy is apparent. No significant signs of tidal disturbances or ongoing mergers are detected. The galaxy appears to be an evolved system with a relatively quiescent star formation rate.
