The galaxy presents as an elliptical morphology, with a smooth, centrally concentrated light distribution. There is a pronounced bulge component, indicated by the concentrated yellow light. The galaxy shows evidence of a disk component. Hints of blue hues are present in the surrounding disk. The edges are blurry. There is no significant presence of dust lanes or spiral arm structures visible in this imaging. There is a sign of possible interactions, the galaxy looks slightly disrupted. 
