The galaxy presents as an elongated spheroid, exhibiting a smooth, centralized concentration of light. The core region is a bright, yellowish-white, suggesting an older stellar population. Progressing outwards, the galaxy shows a gradual decrease in luminosity. There is a subtle color gradient from the core towards the edges, with the periphery exhibiting a slightly bluer hue, which could indicate the presence of some younger stars or ongoing star formation activity, albeit at a low rate. The shape of the galaxy appears mostly undisturbed, with no readily apparent signs of major mergers or significant tidal distortions.
