The galaxy presents a generally smooth and elliptical morphology. Its core exhibits a concentrated, bright, reddish-orange hue, indicative of an older stellar population, while the outer regions display a gradual fading, with greenish-yellow tinges which could indicate recent star formation. The light distribution appears fairly uniform, lacking prominent spiral arms or other distinct features typically associated with disk galaxies. The overall shape is approximately spheroidal with a slight preference to an in-between elliptical shape; it appears largely undisturbed, showing little evidence of ongoing or recent major merger events. There may be minor disturbances, but the overall symmetry suggests a dynamically relaxed system. The estimated size is several kiloparsecs across.
