The galaxy presents a generally smooth and concentrated morphology, suggestive of an elliptical galaxy. The dominant feature is a centrally located bright core, which indicates a region of high stellar density. There is a noticeable decrease in surface brightness moving outward from the core, but no distinct features like spiral arms or a bar are observed. The overall color of the galaxy appears slightly redder, perhaps indicating an older stellar population and lower ongoing star formation. Its shape appears to be more round, showing no major mergers in the recent past. Slight disturbances are likely present.
