The galaxy appears as a relatively smooth, elliptical-like structure with a concentrated central bulge. Its color is predominantly yellowish-white, suggesting an older stellar population with fewer young, massive stars. There is little evidence of spiral arms or a prominent disk. No significant dust lanes or regions of active star formation are visible. The galaxy appears to be quite round and undisturbed, without any signs of major mergers or tidal interactions. The faintness of the galaxy suggests it is at a considerable distance. Overall, it presents the characteristics of a mature elliptical galaxy with a high degree of sphericity and minimal recent star formation.
