The galaxy appears as a centrally concentrated object with a smooth, elliptical morphology. A significant spheroidal component is evident, dominating the overall light distribution. The galaxy exhibits a yellowish-white core, which likely indicates an older stellar population. The outer regions display a gradual decrease in surface brightness, with hints of a slightly flattened shape. There are suggestions of very subtle spiral arm structures in the outer disk, but these are not well-defined, with the classification leaning towards a smooth galaxy. The color gradients suggest a possible radial variation in stellar population, with bluer colors potentially present in the outer regions.