The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a concentrated central bulge with a gradual decrease in luminosity outward. The color profile suggests a predominantly older stellar population, characterized by a yellowish-orange hue. There is little evidence of spiral arm structure or significant dust lanes. The galaxy appears largely undisturbed, showing no clear signs of ongoing mergers or tidal interactions. Its overall structure is consistent with a spheroidal system, likely an elliptical galaxy at an estimated distance implied by its redshift. There are no prominent star-forming regions visible; the galaxy seems quiescent with a very low star formation rate.
