The galaxy presents a largely elliptical morphology, appearing quite smooth and generally featureless. The light is centrally concentrated, exhibiting a bright core that diffuses outward into a more extended halo of fainter light. There is a subtle color gradient, with the core appearing more yellowish-white, suggesting an older stellar population, while the outer regions exhibit a slightly bluer tint, possibly indicating the presence of younger stars, albeit at a lower concentration. Overall, the galaxy exhibits a relatively high degree of rotational symmetry. There are no distinct spiral arms or other prominent features typically associated with disk galaxies visible at this resolution. Minor disturbances in the light profile cannot be ruled out, but no major distortions or tidal features indicative of recent mergers are apparent.
