The galaxy presents an overall elliptical morphology, appearing somewhat elongated. It has a smooth, diffuse appearance without readily discernible spiral arms or a prominent disk structure. The light distribution suggests a concentration of stellar population towards the center, with a gradual decrease in intensity moving outward. The core region exhibits a slightly redder hue, indicative of older stellar populations. Subtle variations in color are present, potentially suggesting regions of varying star formation activity. The overall structure appears relatively undisturbed, with no obvious signs of major mergers or significant tidal interactions. The galaxy presents a fuzzy halo, typical of older systems.
