The galaxy presents as a relatively smooth, elliptical-like structure. Its core exhibits a bright, concentrated luminosity, suggesting a high density of stars in the central region. The light distribution appears largely spheroidal, with a gradual decrease in intensity moving outward from the core. There's minimal indication of spiral arms or distinct features. The galaxy's color profile suggests a population of older stars, with a yellowish hue dominating the overall appearance. No significant dust lanes or regions of active star formation are readily apparent. The galaxy exhibits a compact size and a regular morphology, indicating a relaxed state and mature evolutionary stage.
