The galaxy presents a somewhat smooth, elliptical-like morphology, with a concentrated central bulge that appears nearly spherical. The light distribution is dominated by yellowish hues, suggesting a population of older stars with relatively low ongoing star formation. The overall color is quite red, indicative of an evolved stellar population. The galaxy appears relatively isolated, showing no obvious signs of major recent or ongoing mergers, though some subtle disturbances or extensions of the outer isophotes cannot be ruled out entirely. There might be some disk-like component within the galactic body. The size suggests a considerable galactic body, with a mass on the higher end.
