The galaxy appears as a centrally concentrated object with a smooth, elliptical morphology. It exhibits a gradual decrease in luminosity from the core outwards. The galaxy's overall color profile suggests a population of older stars, based on the higher intensity of red-wavelength light. There is a subtle hint of bluer light in the galaxy's overall emission, which could indicate a low level of ongoing star formation activity. No distinct spiral arms or bar structures are apparent. A slight deviation in the smoothness of the galaxy's halo may point to a minor tidal disturbance or past merger event. The shape is close to round, but slightly elongated, with an average size for galaxies at its distance.
