The galaxy presents as a relatively smooth, elliptical structure, exhibiting a high degree of central concentration of light. The central bulge appears bright and yellow-white, indicating a population of older stars. Moving outward from the center, the light gradually decreases in intensity, with the outer regions appearing less defined and more diffuse. There is a slight flattening, giving it a somewhat elongated shape. There's no clear evidence of spiral arms or prominent dust lanes. It shows no signs of major merging events, although some minor disturbances cannot be ruled out. The color gradient suggests that star formation is suppressed throughout the majority of the galaxy.