The galaxy presents as a relatively smooth, elliptical-like structure, with a concentrated central bulge. There is an absence of clearly defined spiral arms or a prominent disk. The galaxy exhibits a gradual decrease in luminosity from the core outwards. The color appears consistent across the visible structure, without significant variations that might suggest distinct stellar populations or active star-forming regions. There is no evident sign of tidal disturbances, merging activity, or interaction with other galaxies. The overall morphology suggests an evolved system, possibly an elliptical galaxy or a lenticular galaxy viewed face-on, with minimal ongoing star formation.
