The galaxy presents a largely elliptical morphology, appearing quite smooth and centrally concentrated with little visible substructure. The core exhibits a bright, yellowish-orange hue, suggesting an older stellar population likely dominated by red giants and relatively low ongoing star formation. This core region gradually fades into a more diffuse halo, exhibiting faint blue tinges at the outermost edges. These subtle blue colors indicate the presence of younger, hotter stars, possibly resulting from minor recent star formation activity in the galactic periphery. The galaxy displays a high degree of rotational symmetry, appearing almost perfectly round. There is no clear evidence of significant tidal distortions, ongoing mergers, or major disturbances in the overall morphology. Small disturbances cannot be completely ruled out, but they are faint, if present at all.
