The galaxy presents as a centrally concentrated, somewhat smooth object. Its overall shape appears to be elliptical or lenticular, with a slight elongation, rather than exhibiting spiral arm structures. The core region is bright and unresolved, likely indicative of a high stellar density or an active galactic nucleus. The surrounding halo or outer region of the galaxy exhibits a subtle color gradient, transitioning from a bluer hue in the inner regions to a redder tint towards the outer edges. This may suggest variations in stellar populations, with younger, bluer stars dominating the central region and older, redder stars populating the periphery. There's a subtle suggestion of some faint features, potentially indicating a weak disk or tidal disturbances, but its overall smoothness suggests a galaxy that has largely completed its formation or has undergone significant mergers in the past.
