The galaxy presents a largely smooth and elliptical morphology. The central region exhibits a high concentration of light, appearing as a bright, yellowish-white core. This concentrated core diffuses outwards, transitioning into a less luminous halo. The overall color is notably redder, suggesting an older stellar population dominating the galaxy's light output. There is little to no evidence of spiral arm structure or active star formation regions visible in this image. The galaxy appears relatively undisturbed, with no signs of major mergers or tidal interactions. A slight elongation in the galaxy's shape is noticeable, but it maintains an overall rounded form.
