The galaxy presents a largely smooth, elliptical morphology. The central region exhibits a concentrated, bright yellowish-orange hue, suggesting a population of older stars. The light becomes less concentrated, transitioning to a redder tone with increased distance from the center, still indicating a dominant older stellar population. There is a slight indication of a blue light, which can be an indication of star formation. The overall appearance of the galaxy is regular, showing little evidence of significant disturbances or mergers. The galaxy's roundness is quite pronounced.
