The galaxy presents as a relatively smooth, centrally concentrated object. Its overall shape is generally round, showing minimal deviation towards a flattened or elongated form. There is no obvious spiral arm structure or prominent disk. The light distribution is fairly even, with a smooth gradient increasing towards the center. The central region is a bright, concentrated core. The colors indicate a population of older stars. There is very little visual evidence of ongoing star formation or significant dust obscuration. Based on its morphology, this galaxy is likely an elliptical.
