The galaxy presents a generally smooth, elliptical morphology. It appears largely featureless upon visual inspection, lacking any discernible spiral arm structures or significant dust lane obscuration. The light distribution is concentrated towards the center. The color indices suggest a population of older stars, exhibiting a redder hue. There is no evidence of major ongoing mergers, but minor tidal disturbances cannot be ruled out. Overall, it is a moderately luminous, relatively massive galaxy with a low star formation rate and lies at a considerable distance. Its light is dominated by an evolved stellar population.
