The galaxy appears as a single, concentrated body with a generally smooth profile. It exhibits a near-spherical morphology, with minimal deviation from a circular shape. The galaxy's core presents a bright, concentrated luminosity, which gradually diminishes towards the outer edges. The color profile suggests a predominantly older stellar population, with a yellowish-orange hue dominating the overall color. There is minimal evidence of spiral arm structures or significant dust lanes, and no immediately apparent signs of ongoing major merger activity or significant tidal disturbances. The galaxy appears relatively undisturbed.
