The galaxy presents as an elliptical or lenticular type with a smooth, concentrated central bulge. It exhibits a relatively high degree of rotational symmetry, appearing mostly round in shape, with a slight elongation. The galaxy lacks prominent spiral arm structures, with only subtle indications of disk features. Its color profile suggests an older stellar population, with a yellowish or redder overall hue indicating lower rates of current star formation. There appears to be no major ongoing merging activity, with the general morphology undisturbed, although minor disturbances cannot be ruled out. The size is typical for a galaxy at its redshift.
