The galaxy presents as a centrally concentrated elliptical type, exhibiting a relatively smooth and homogenous light distribution. The morphology suggests a relatively evolved system with minimal discernible substructure. The core region appears quite bright, transitioning to a fainter halo with less distinct boundaries. The color profile indicates a redder hue, suggesting an older stellar population with lower star formation activity. There may be a slight hint of asymmetry, but its significance is difficult to assess given the image resolution. The overall appearance is consistent with a massive galaxy residing at a considerable cosmological distance.
