The galaxy presents a largely smooth, elliptical morphology. The central region exhibits a strong concentration of light, indicative of a substantial stellar population and potentially a supermassive black hole. The galaxy appears to have a substantial mass. Fainter, less defined, asymmetrical features or diffuse extensions extend from the primary body. A hint of spiral arm-like structures can be observed. The light distribution shifts from yellower in the core to greener colors outwards indicating an increased presence of younger, bluer stars in the outer regions. There is no evidence of significant ongoing mergers or major disturbances from interactions with other galaxies.
