The galaxy presents a centrally concentrated, elliptical morphology with a smooth light profile. The core exhibits a bright, yellowish-white hue, indicative of a high density of older stellar populations. Moving outward from the core, the color transitions subtly to a redder shade, still maintaining a relatively homogenous appearance without prominent spiral arm structures or dust lanes. The outer regions fade gradually into the background sky, suggesting a lack of significant tidal disturbances or recent major mergers. The galaxy’s overall shape appears slightly elongated rather than perfectly circular. The galaxy appears as a large, relatively massive system in the universe. Overall, the system appears as a relatively old, relaxed galaxy, likely past its peak star formation epoch, with a substantial population of evolved stars.
