The galaxy presents as an elliptical or lenticular morphology, exhibiting a smooth, concentrated light profile. It possesses a central bulge that dominates the galaxy's overall structure, with a noticeable decrease in surface brightness as we move outward from the core. The color indices suggest a population of older stars. There is little evidence of active star formation or prominent spiral arm structures. Faint hints of a disk may be present, but the galaxy is predominantly spheroid-shaped. No signs of major mergers or significant tidal disturbances are immediately apparent; the galaxy appears relatively undisturbed in its present state. The overall impression is that of a passively evolving system with a substantial stellar mass.
