The galaxy presents as a centrally concentrated, smooth object, likely an elliptical galaxy or a lenticular galaxy seen face-on or at a slight inclination. The light profile appears relatively uniform with a bright core, suggesting an older stellar population dominates. There is a slight elongation, deviating from a perfectly circular shape. No distinct features such as spiral arms or dust lanes are readily apparent. There is little evidence of significant recent star formation activity within the observable region. The overall structure indicates a well-established, dynamically relaxed system.
