The galaxy appears to be a relatively smooth, elliptical type. It has a bright, centrally concentrated bulge, emitting strongly in the yellow-red wavelengths, possibly indicating an older stellar population. The galaxy presents an overall elliptical shape, showing a high degree of central concentration with a small, subtle deviation in the symmetry. Hints of redder regions are visible, possibly areas of dust obscuration or active star formation, though these appear subdued. There is no clear evidence of strong spiral arm structure, but instead, there are low-contrast asymmetric shapes surrounding the center of the galaxy. Based on the color, this is likely a galaxy where star formation has slowed down or stopped, resulting in primarily older, redder stars and little to no blue/purple light. The morphology suggests it is in an intermediate stage of its evolution. The light detected is faint, which is expected as it's at a high redshift.
