The galaxy presents a flattened, elliptical morphology with a smooth appearance. The central region exhibits a high concentration of light, suggesting a prominent bulge. The galaxy displays a color gradient, transitioning from a yellowish-white core to a bluer outer disk. This likely indicates older stellar populations concentrated within the bulge, and younger populations in the outer regions. The ellipticity of the galaxy is substantial, indicating a significant deviation from a spherical shape. There are no readily apparent spiral arm structures or dust lanes visible in this image. Overall, the galaxy appears to be a relatively evolved system, with a substantial fraction of its stellar mass concentrated within the central bulge.
