The galaxy presents as a relatively smooth, elliptical-like structure with a high degree of central concentration. The core region exhibits a bright, concentrated luminosity, with a slightly reddish hue suggestive of an older stellar population. The surrounding halo gradually diffuses outwards, decreasing in brightness. There's a faint hint of a disk-like morphology with a very slight blue tinge. There is no visible spiral arm structure and no signs of any major mergers or tidal disturbances. Overall, the galaxy appears relatively undisturbed and evolved.
