The galaxy presents a largely smooth and elliptical morphology, lacking any clear spiral arm structure. The central region exhibits a strong concentration of light, appearing bright and yellowish-orange in color. This suggests an older stellar population dominates the core. Moving outwards from the core, the light gradually diminishes, forming a diffuse halo of stars. The overall shape is somewhat elongated, but without any noticeable distortions that would indicate a recent or ongoing merger event. The galaxy's color suggests minimal recent star formation.
