The galaxy presents a largely smooth morphology, with minimal apparent features such as spiral arms or a distinct disk. The central region exhibits a concentrated, bright core that diffuses outwards into a more extended halo. The galaxy appears elliptical in shape, with an observed roundness, showing no obvious signs of significant tidal distortions or major merger events. Minor disturbances can not be ruled out due to the image quality. The galaxy's color profile suggests a population of older stars, with a reddish-yellow hue dominating the overall light emission, with some green coloration.