This galaxy presents as an elliptical type, exhibiting a generally smooth, featureless morphology. There is a concentration of luminosity towards the central region. The shape is somewhat elongated, with the luminosity distribution appearing more diffuse outwards from the core. The color profile suggests a population of older stars, exhibiting light in the green, red, and blue wavelengths. There is no prominent indication of recent or ongoing major mergers or tidal disturbances. The galaxy shows no apparent spiral arm structure or significant dust lane obscuration.
