This galaxy presents as a centrally concentrated, smooth object. Its morphology is largely spheroidal, appearing mostly round with a slight deviation towards an intermediate shape. The galaxy exhibits a prominent bulge, characterized by a yellow-orange hue, suggesting a population of older stars and relatively low star formation activity. No distinct spiral arm structures or prominent dust lanes are discernible. There is no major visual evidence of ongoing or recent major mergers or tidal disturbances. The smooth profile and concentrated light distribution indicate that this is likely a relatively massive system with a well-established stellar population.
