The galaxy exhibits a generally smooth, elliptical morphology, appearing mostly round in shape. There is a distinct central bulge that is bright and concentrated. Moving outward from the core, the light gradually fades into a more diffuse halo. No prominent spiral arm structures or dust lanes are visible. The overall color suggests an older stellar population, with a yellow-red hue dominating the galaxy's light. Indications of very low star formation can be inferred from the lack of blue light and the smooth texture. No apparent signs of recent or ongoing mergers or tidal disturbances are detected.
