The galaxy presents as a luminous elliptical form, exhibiting a smooth, diffuse light profile. The central region displays a concentrated core of intense brightness, suggesting a high density of stars and potentially a supermassive black hole at its nucleus. Moving outwards from the core, the light gradually diminishes, forming an extended halo that lacks any apparent spiral arms or distinct features. There may be subtle irregularities in the outer regions of the halo, possibly indicating minor gravitational interactions or past merger events. The galaxy appears slightly elongated, but is mostly rounded. In terms of color, the galaxy exhibits a predominantly reddish hue, particularly concentrated in the core. This indicates a population of older, cooler stars. The outer regions are comparatively bluer, which may be related to a younger stellar population or recent star formation activity, albeit at a low rate.
