The galaxy appears as a centrally concentrated system with a smooth, diffuse profile. A prominent, bright nucleus is visible, suggestive of an active galactic nucleus or a high concentration of stars. There are hints of a faint, extended halo or disk surrounding the core, although the low surface brightness makes it difficult to discern distinct structures. Overall, the galaxy presents a spheroidal morphology, with a lack of spiral arms or significant irregular features. The color gradient indicates a potentially older stellar population.
