The galaxy presents as a relatively compact object, exhibiting a largely smooth and centrally concentrated morphology. It appears as an elliptical or lenticular galaxy at a moderate redshift. There is a noticeable color gradient with bluer hues towards the center and redder hues towards the periphery. This suggests a population of younger, hotter stars concentrated in the central regions, possibly indicating recent or ongoing star formation, or a dusty nucleus. A small amount of asymmetry or faint tidal feature suggests the possibility of past minor merger events.
