The galaxy presents as a centrally concentrated, smooth structure with a slightly elongated morphology. The core exhibits a bright, diffuse glow that fades gradually outward. There is minimal discernible detail within the galaxy; no spiral arms or distinct features are readily apparent. The overall color appears to be a bluish-white hue, indicating a possible presence of relatively young, hot stars, though this is somewhat subdued. There is faint asymmetry to the outskirts, hinting at potential minor gravitational disturbance. No significant dust lanes or signs of active star formation are obviously present. The galaxy appears to be a relatively isolated system.
