The galaxy presents as a centrally concentrated system with a smooth, elliptical morphology. The core exhibits a bright, relatively uniform luminosity. The isophotes appear somewhat elongated, suggesting a deviation from perfect circularity. There's a subtle color gradient visible; The central region has a more yellowish hue that could be older stars, while the outer regions appear marginally bluer, indicating the presence of younger stellar populations. The absence of distinct spiral arms or prominent dust lanes indicates a lack of significant recent star formation. The overall appearance is consistent with a mature galaxy, potentially in the process of, or already having undergone quenching.
