The galaxy appears as a relatively compact and smooth structure. Its morphology indicates a spheroid shape, with a high degree of roundness and minimal evidence of a disk-like structure. The light distribution suggests an elliptical or lenticular galaxy type. There is no visible indication of spiral arms or significant dust lanes. The galaxy shows no obvious signs of ongoing merging activity or major disturbances, maintaining a fairly regular and undisturbed appearance. The light profile appears relatively uniform, lacking distinct features or significant color gradients, suggesting a more homogenous stellar population. Overall, the galaxy appears to be a well-formed, quiescent system at a moderate redshift.
