The galaxy presents as a largely smooth, elliptical structure. The core exhibits a bright, concentrated luminosity, appearing yellowish in color, which suggests a population of older stars. Moving outward from the core, the light gradually fades and transitions to a more bluish hue, implying the presence of a younger, bluer stellar population in the outer regions, possibly indicating ongoing or recent star formation. The overall morphology does not show any signs of significant disturbances or major tidal interactions, it appears relatively undisturbed and relaxed. The galaxy’s shape is intermediate between round and elongated. No prominent spiral arms or other distinct features are discernible.
