The galaxy presents a generally elliptical morphology with a high degree of smoothness. The central region exhibits a bright, concentrated core. There is a noticeable color gradient, trending from yellow-white in the core to slightly redder hues in the outer regions, indicating the presence of older stellar populations with very little recent or current star formation.

No distinct spiral arm structures or prominent dust lanes are discernible. There are no significant signs of tidal disturbances or ongoing mergers within the observable light. It's structure is mostly rounded with some slight elongation.
