The galaxy presents a generally smooth and rounded morphology, appearing relatively undisturbed. There is evidence of a disk-like structure but it is not well defined. There is a bright central bulge, which appears to dominate the galaxy's luminosity. The overall color is bluish-white, suggesting the presence of a population of younger, hotter stars. The galaxy does not exhibit any obvious signs of ongoing major mergers, though some minor tidal features or disturbances cannot be ruled out. There is a possibility of minor interactions.
