This galaxy presents as an elliptical morphology, exhibiting a high degree of central concentration. The light profile suggests a smooth, spheroidal distribution of stars, with a lack of discernible spiral arm structures or prominent dust lanes. The core of the galaxy is bright and yellowish-white, indicating a population of older stars dominating the central regions. Moving outwards from the core, the color transitions towards a slightly bluer hue, suggesting a more mixed stellar population, or perhaps a minor amount of ongoing star formation in the outer regions. Overall, the galaxy exhibits a relaxed, undisturbed appearance, lacking any obvious signs of recent major mergers or tidal interactions. Faint extensions of light surround the main body of the galaxy and may be a halo.
