The galaxy presents as a relatively well-defined elliptical structure, characterized by a smooth, centrally concentrated luminosity profile. The core exhibits a bright, yellowish-white hue, suggestive of a population dominated by older stars. Moving outwards from the core, the galaxy displays a bluer color gradient, hinting at the presence of a younger stellar population in the outer regions or ongoing star formation. There's a subtle indication of a flattened disk component. The overall morphology suggests a relatively undisturbed system, although a minor interaction or past merger event cannot be completely ruled out.
