The galaxy presents as a relatively smooth, elliptical structure. There is minimal discernible spiral arm structure or prominent dust lanes. The central bulge appears bright and well-defined, with a gradual decrease in luminosity towards the outer regions. The overall color profile appears consistent, with a subtle reddening towards the central region, potentially indicative of an older stellar population concentration. The galaxy exhibits an intermediate ellipticity, neither perfectly spherical nor highly elongated. Faint disturbances may exist within the overall structure, although this could be visual noise within the image. There is no obvious large scale major ongoing merger.
