The galaxy presents as a centrally concentrated, largely smooth light distribution. The overall shape appears elliptical or spheroidal, with a high degree of circularity. There's no obvious disk structure or spiral arm morphology visible in this image, suggesting it is a relatively undisturbed system. The galaxy exhibits a color gradient, with a slightly bluer hue in the outer regions, transitioning to a redder core. The color variation suggests some ongoing star formation activity, albeit at a lower rate, with a higher concentration of older stellar populations in the central bulge. There are no apparent signs of major mergers or tidal disturbances in the immediate vicinity of the galaxy, although some faint, minor disturbances cannot be completely ruled out.
