This galaxy exhibits a generally elliptical morphology, appearing somewhat flattened in the image. The central region displays a bright, concentrated core. The overall color profile suggests a population of relatively old stars. The edges show some irregularity, potentially indicating a minor interaction or disturbance, though the main body appears largely undisturbed. No distinct spiral arm structure is apparent, nor is there evidence of a major ongoing merger. The galaxy exhibits a diffuse halo.
