The galaxy presents a relatively smooth, elliptical morphology, appearing largely featureless at this resolution. Its central bulge is prominent, displaying a concentrated luminosity with a yellowish-orange hue, suggesting an older stellar population. A faint, diffuse halo surrounds the core, showing a gradual decrease in surface brightness with increasing radial distance. Subtle color variations are present in the outer regions, hinting at possible pockets of younger, bluer stars, although the dominant color profile indicates a galaxy dominated by evolved stars. There is no obvious evidence of spiral arm structure or significant dust lanes. The overall appearance suggests a system that has largely completed its major star formation phase, now undergoing a more quiescent period of stellar evolution.
