The galaxy exhibits a generally elliptical morphology, appearing largely smooth and featureless in this image. There is a subtle color gradient visible, transitioning from a more yellow-white central region to a slightly redder outer halo. This color shift could indicate a change in stellar population, with older, redder stars dominating the outer regions, and younger, hotter stars concentrated centrally.

The round appearance suggests the galaxy is an elliptical, but not perfectly spherical. There is no obvious disk structure visible, based on the lack of spiral arms or a flattened shape. There is a hint of what might be minor structural disturbance in the very outer edges of the galaxy; It could be indicative of a past interaction or merger event, though this feature is not well defined. Overall the light is relatively concentrated towards the center suggesting the galaxy's structure is well formed.
