The galaxy appears as a relatively smooth, elliptical-shaped object. Its central region exhibits a bright, concentrated luminosity, suggesting a dense stellar population or possibly an active galactic nucleus. The galaxy displays a color gradient, shifting from a yellowish-white core to a subtly bluer outer halo. This color variation could indicate differing stellar populations, with older, redder stars concentrated in the center and younger, bluer stars present in the outer regions, though the overall color suggests an older stellar population dominates. There is little evidence of spiral arm structure or significant dust lanes. The outer edges appear diffuse, fading gradually into the background sky.
