The galaxy presents a predominantly smooth, elliptical morphology with a high degree of central concentration. The core exhibits a bright, yellowish-white hue, possibly indicating a population of older, evolved stars. Moving outward from the core, the color transitions to a slightly bluer tint. This change in color suggests a possible presence of some younger stars or subtle dust features in the outer regions, though these are not distinctly resolved in the image. The overall shape appears nearly round, lacking any obvious spiral arms or strong bar structures. There are no clear signs of major mergers or significant tidal disturbances visible, the galaxy appears relatively undisturbed. 
