The galaxy presents a smooth, elliptical morphology. Its core exhibits a bright, concentrated luminosity, suggesting a high density of stars in the central region. Moving outward from the core, the light gradually diffuses, indicating a diminishing stellar density. The overall shape is generally round. There is little indication of spiral arms or other distinct structural features commonly observed in spiral galaxies. Faint blue tinges are observed in the out parts of the galaxy, which suggest low levels of recent or ongoing star formation. There is no visible distortion.
