The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a centrally concentrated light profile, with a gradual decrease in luminosity moving outwards from the core. The core region shows a yellowish hue, which may indicate an older stellar population. The outer regions of the galaxy appear slightly bluer, potentially indicating regions of more recent, low-level star formation activity. There is no clear evidence of spiral arms, bars, or other distinct features. Overall, it seems to be a typical elliptical galaxy at an intermediate redshift. The shape is moderately elliptical, appearing neither perfectly round nor significantly elongated. No major disturbances from mergers or interactions are obviously visually present.
