The galaxy presents a largely smooth morphology. The light profile appears centrally concentrated, with a high degree of roundness. The core exhibits a yellowish hue, potentially indicating an older stellar population or significant dust obscuration. Moving outwards from the core, the galaxy transitions to a fainter, bluish halo or disk. The overall structure shows no obvious signs of major disturbances or ongoing mergers, although subtle features might be present at a resolution beyond the limitations of this image. Star formation seems to be moderate.
