The galaxy presents as a relatively smooth, elliptical morphology. There is little visible evidence of spiral arms or significant disk-like structures. The galaxy appears largely spheroidal, with a high degree of central concentration. The color profile suggests an older stellar population, dominated by redder wavelengths. The galaxy is very round in shape with no visible distortions due to mergers or interactions. Its absolute magnitudes appear to be quite high and its star formation rate is quite low. The light is centrally concentrated, indicative of an elliptical galaxy morphology.