The galaxy presents a largely smooth, elliptical morphology. Its shape appears close to spherical, with minimal discernible disk-like features. There's a subtle central concentration of light, fading gradually towards the outer edges. No spiral arms or bar structures are apparent. The light distribution suggests a relatively old stellar population, with a dominant reddish hue. Minimal signs of dust lanes or prominent star-forming regions are visible, indicating low ongoing star formation activity. There is little evidence to suggest recent or ongoing major mergers, although there may be subtle distortions indicating minor past interactions. Overall, it appears to be a relatively quiescent, evolved system.
