The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a bright, yellowish-white core that likely indicates an older stellar population. The surrounding halo shows a gradual decrease in luminosity, appearing more diffuse and slightly bluer in color than the core. This hints at the presence of some younger stars in the outer regions, though they are not particularly prominent. No obvious spiral arms or other distinct features are discernible. The overall shape appears largely spheroidal, with a high degree of roundness, suggesting an elliptical morphology. There is no clear indication of any major merger events or significant tidal disturbances in its structure.
