The galaxy presents as a luminous, well-defined spheroid with a generally smooth texture. Its color is predominantly yellowish-orange, which suggests an older stellar population. The galaxy exhibits a high degree of central concentration, with light intensity diminishing gradually from the core towards the periphery. It is estimated to be roughly 5.6 kpc in radius. I do not see any spiral arm structures or significant dust lanes present. The overall morphology appears undisturbed, indicating a lack of recent major mergers or interactions. Given its redshift, this is a massive galaxy with a very low specific star formation rate.
