The galaxy presents as a luminous, reddish-orange object. Its overall form appears relatively smooth and concentrated towards the center, suggesting a high degree of internal order. The light distribution indicates a structure somewhere between a perfect sphere and a flattened disk, with more of an in-between shape. There is a possibility of some disturbance in its form, potentially indicating a past interaction, though no strong evidence of a merger can be seen. The galaxy is likely quite massive with moderate star forming activity.
