The galaxy presents as a centrally concentrated object. It has an overall smooth appearance, with a round morphology that indicates it might be an elliptical galaxy. The color gradient shifts from a bluer hue in the center to redder hues in the outer regions, potentially indicating older stellar populations towards the galaxy's periphery. There are no strong indications of spiral arms or significant dust lanes. Faint distortions may be present but are not conclusive, potentially indicating minor gravitational interactions or internal structures. The object is relatively compact, exhibiting a degree of symmetry about its core.
