The galaxy presents as a centrally concentrated system with a moderate degree of overall smoothness. It exhibits a flattened, elliptical morphology, appearing more oblate than perfectly spherical. The central region displays a bright, concentrated core, suggesting a high stellar density. A subtle, extended halo surrounds the core, gradually fading into the background. There's a hint of faint, diffuse structure within the halo, indicating possible tidal features or minor disturbances, though no major merger events are immediately apparent. The overall color profile is predominantly bluish-white, indicative of ongoing or recent star formation, with a notable contribution from younger, hotter stellar populations. No distinct spiral arms or bar structures are visible.
