The galaxy presents as a centrally concentrated system with an overall elliptical morphology. It exhibits a smooth light distribution, with the majority of its light concentrated in the central bulge region. The bulge displays a yellowish-white hue, potentially indicative of an older stellar population. Fainter, bluer light extends outwards from the central region, suggesting the presence of younger stars or ongoing star formation in the galaxy's outer regions. Hints of reddish hues appear along the edges of the galaxy, possibly indicating regions of dust obscuration or older stellar populations. No distinct spiral arm structures or prominent dust lanes are visible. The galaxy shows no signs of major mergers or significant tidal disturbances. The observed properties are generally consistent with an elliptical galaxy at moderate redshift.
