The galaxy presents a generally smooth, elliptical morphology, with a high degree of central concentration. There is a subtle color gradient from the core outwards, suggestive of differing stellar populations, with a bluer component at the galaxy's outskirts. The galaxy is not perfectly spherical, appearing slightly elongated. There is some evidence of minor disturbances to the galaxy's overall structure, possibly indicating a past or ongoing minor interaction. Overall, the galaxy does not show any major structural distortions or signs of a recent major merger.
