The galaxy presents an overall elliptical morphology, appearing largely smooth in structure with a high degree of central concentration. The core exhibits a distinct yellowish-orange hue, suggesting a population of older stars dominating this region. Moving outwards from the center, the galaxy displays a gradual fading in color, transitioning to a bluer periphery. This likely indicates a younger stellar population in the outer regions, possibly resulting from recent or ongoing star formation activity, however, it is not distinctly visible. The overall appearance indicates a significant mass and is relatively undisturbed, showing no major signs of tidal interaction or ongoing merger events, although it could be classified as showing minor disturbances. The galaxy's structure appears predominantly rounded and lacks any elongated or cigar-shaped distortion.
