The galaxy presents as a relatively compact, centrally concentrated object. It appears to be largely spheroidal in shape, though there may be some slight deviation from perfect roundness. There is some visible color variation within the galaxy. The central region exhibits a yellowish hue, possibly indicating an older stellar population. The outer regions appear somewhat redder. This color variation could be due to differential star formation history. The galaxy is quite luminous, suggesting a significant stellar mass. Star formation is present but is not particularly vigorous. There is evidence of a potential interaction or merger event. Overall, the galaxy presents as a moderately massive elliptical or lenticular galaxy at intermediate redshift with subtle features suggesting recent or ongoing dynamical activity.
