The galaxy presents as a largely smooth, elliptical-like structure with a concentrated central bulge. There's a subtle color gradient observable, with a yellowish-white core gradually transitioning to a bluish halo. The overall morphology suggests a relatively evolved system, possibly with a lower rate of active star formation compared to younger, spiral galaxies. While appearing mostly undisturbed, closer inspection hints at subtle irregularities in the outer regions, possibly indicative of minor gravitational interactions or past merger events. The round and smooth characteristics suggests that the observed system is likely a large mass, early-type galaxy.
