This galaxy appears to be a relatively smooth, elliptical system. It presents with a high degree of central concentration, exhibiting a bright, yellowish core that fades gradually towards the outer edges. The isophotes appear mostly round. There is a subtle hint of asymmetry. Faint, diffuse extensions are visible in the outer regions, but no prominent spiral arms or distinct dust lanes are discernible. The overall color suggests a population of older stars, potentially indicative of lower recent star formation activity.
