The galaxy appears to be a relatively smooth, elliptical galaxy with a high degree of central concentration. The galaxy exhibits a distinct, bright core with a diffuse halo that fades into the background. The shape is generally rounded, though slightly elongated along one axis, suggestive of an intermediate ellipticity. There's minimal evidence of spiral arm structure or distinct dust lanes. Color gradients indicate the presence of a redder stellar population in the central regions, possibly older stars, with hints of bluer regions in the outer parts. The overall visual impression suggests an evolved system, potentially with little ongoing star formation. There is no apparent interaction or merger activity readily visible in the image.
