The galaxy appears to be a relatively luminous object at a considerable distance, based on the observed colors and estimated redshift. Morphologically, it presents a smooth appearance, suggesting a lack of significant spiral arms or other distinct features. The shape is generally rounded, with perhaps a slight elongation or departure from perfect circularity. There is a central concentration of light that fades gradually outwards, suggesting a centrally dense stellar population. The galaxy's overall color is slightly red, hinting at an older stellar population, but there are signs of star formation as well. There is no obvious major merger activity visible, though subtle disturbances may be present.
