The galaxy presents a largely smooth morphology. The central region is significantly brighter and yellowish-white in color, suggesting a concentration of older stars. Moving outwards, the galaxy fades gradually into the surrounding background, with the outer regions exhibiting a slightly bluer hue, indicative of some ongoing star formation, albeit at a low rate. The galaxy appears roughly circular, showing a slight deviation towards an elliptical shape. There are no clear signs of spiral arms or a prominent disk structure, nor any indications of major mergers or strong tidal disturbances. Subtle color variations suggest a non-uniform stellar population distribution.
