This galaxy presents as a fairly smooth object with an elliptical morphology. There is no discernible spiral arm structure or bar feature evident. The light is concentrated towards the center of the galaxy with intensity tapering off with increasing radius. It appears mostly spheroidal with a slight deviation from perfect circularity. The color profile suggests a population of older stars, visible through the predominantly yellow hue of the galactic core. Faint blue regions are present in some areas, indicating the presence of some younger stars. There does not appear to be any major ongoing merger activity or tidal disturbance of the galaxy.
