The galaxy presents as a slightly extended object, though the resolution limits detailed morphological assessment. The light profile appears relatively smooth, with no obvious spiral arm structures or a distinct central bulge discernible. The color of the galaxy appears to be slightly redder, suggesting the presence of an older stellar population or significant dust obscuration. There is a hint of faint, diffuse emission surrounding the central region. The Z band magnitude is infinity, suggesting this galaxy is highly redshifted or is not emitting energy in the Z band. Based on these observations, this could be an elliptical galaxy at a significant distance. There is the possibility it has undergone some past disturbances, which is making the light more red.
