The galaxy appears to be an elliptical galaxy at a considerable distance. It exhibits a smooth, relatively featureless morphology with a concentrated central bulge that is yellowish-white, suggesting an older stellar population. There is a clear radial decline in surface brightness from the core to the outer regions. The galaxy appears mostly homogenous in color and texture, without any distinct spiral arms, bars, or dust lanes visible. A subtle extension of the light distribution suggests a slight deviation from perfect ellipticity, possibly indicating a minor tidal interaction or past merger event. The overall structure suggests a well-mixed stellar population, indicative of a dynamically evolved system. It is compact in angular size, which, in combination with its estimated redshift, indicates it is a physically large and luminous galaxy. There are no obvious indications of significant ongoing star formation activity based on the lack of blue colors.
