The galaxy presents as a centrally concentrated, smooth structure with a generally round morphology. Its light profile suggests a relatively undisturbed system with minimal asymmetry. The galaxy exhibits a dominant bluish hue, with a hint of green, concentrated towards its core, indicating the presence of younger, hotter stellar populations and potentially ongoing or recent star formation. There is a subtle color gradient suggesting a slightly redder outer region, which may indicate an older stellar population as we move away from the core. No distinct spiral arms or prominent dust lanes are discernible. The image suggests a massive galaxy at a considerable distance, consistent with a system at redshift z ~ 0.386, implying a lookback time of approximately 4.7 billion years.
