The galaxy presents a generally smooth, elliptical morphology. The light is concentrated towards the center, with a radial falloff in surface brightness. The galaxy appears to be largely spheroidal in shape, displaying a high degree of circular symmetry and no apparent spiral arm structures or strong irregularities. The color is primarily yellowish-orange, suggesting a population of older stars. This color indicates relatively low levels of current star formation. The size of the galaxy is moderate, with no apparent signs of ongoing major mergers or significant tidal interactions. There may be faint indications of a minor disturbance in the surrounding halo.
