The galaxy presents as a centrally concentrated object with a largely smooth morphology. A dominant, bright, yellowish-white core is evident, suggesting a substantial population of older stars. The overall shape appears elliptical or spheroidal, with a slight elongation. The galaxy exhibits a gradual decrease in luminosity moving outward from the core, transitioning into a fainter, bluer halo-like region. There are no easily discernible spiral arms or prominent dust lanes visible, indicating a lack of significant current star formation activity. Faint irregular features in the outer region may suggest past minor interactions or disturbances. The color gradient indicates a change in stellar population from old stars in the core to a younger population on the outskirts.
