This galaxy presents as a flattened, elongated structure, likely a disk galaxy viewed at a significant angle. The central region exhibits a concentrated, bright yellowish-white luminosity, suggesting a substantial population of older stars and potentially a supermassive black hole actively accreting material at its core. The outer regions of the galactic disk show a faint, bluish-green hue, indicating the presence of younger, hotter stars and ongoing star formation. There are no clearly discernible spiral arm structures, and the morphology appears relatively smooth. The overall shape suggests this galaxy is an elliptical or lenticular galaxy rather than a spiral galaxy. No major disturbances or tidal features are apparent, indicating a lack of recent major merger events. The color gradient from the core outwards suggests a radial variation in stellar population and star formation activity.
