The galaxy presents a largely smooth, elliptical morphology. Its color profile indicates a concentration of older stellar populations, exhibiting a yellowish-orange hue that intensifies towards the galactic center. There is some subtle evidence of a flattened shape, though it appears mostly spheroidal. There are hints of a faint, extended halo surrounding the central body, though the image resolution makes precise delineation difficult. No spiral arm structures are visibly apparent, and there are no clear signs of significant ongoing star formation as indicated by a lack of bright blue regions. There is no indication of major mergers or disturbances. The galaxy appears relatively isolated, with no obvious close companion galaxies or tidal features in the surrounding area.