The galaxy presents as an elliptical morphology, displaying a smooth, centralized concentration of light. The overall shape appears elongated, leaning towards a cigar-like structure. The light distribution suggests a largely featureless stellar population, lacking distinct spiral arm structures or prominent dust lanes. A color gradient is observed, shifting from a yellowish-orange hue in the core to a slightly bluer tone in the outer regions, hinting at some degree of ongoing star formation. No indications of significant tidal disturbances or ongoing merger activity are apparent, indicating a relatively undisturbed system. The overall appearance is consistent with a massive galaxy with a substantial stellar mass.
