The galaxy presents as an elliptical morphology. It has a relatively smooth appearance, lacking prominent spiral arms or significant dust lanes. The color profile suggests a dominant population of older stars, exhibiting a yellowish hue. The central region appears brighter and more concentrated, indicative of a dense stellar core, which potentially harbors a supermassive black hole. There are hints of lower levels of star formation activity within the galaxy. Overall, the galaxy seems to be a well-formed elliptical galaxy at intermediate redshift.
