The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology appears largely elliptical with a high degree of roundness. There is a distinct color gradient, with the core exhibiting a yellowish-white hue, suggesting an older stellar population dominating the central region. The outer regions display a slightly bluer tint, hinting at the presence of some younger stars or ongoing, albeit subdued, star formation. There is no clear evidence of spiral arms or a prominent disk structure. The overall impression is that of a mature, relatively quiescent system with minimal signs of recent major mergers or significant tidal disturbances.
