The galaxy presents as a centrally concentrated object with a generally smooth morphology. There is a slight elongation in its overall shape, but the deviation from perfect circularity appears minimal. The light profile suggests a relatively quiescent system, lacking distinct spiral arms or prominent star-forming regions. A subtle color gradient is observed, with the central region exhibiting a more yellowish hue, potentially indicative of an older stellar population. The outer regions show a slight bluer tint, hinting at the presence of some younger stars, although less pronounced. There is no obvious evidence of ongoing or recent major mergers or tidal disturbances. The overall appearance is consistent with an elliptical or lenticular galaxy at the observed redshift.
