The galaxy appears to be a luminous, elliptical system with a smooth, centrally concentrated light distribution. Its overall color index suggests a relatively evolved stellar population, potentially dominated by older stars. The system exhibits a moderate degree of roundness, with no obvious spiral arm structures or bar features discernible in the observed wavelengths. There is a hint of a minor perturbation in the isophotes which may indicate an interaction or recent merger. No obvious dust lanes or signs of active star formation are immediately apparent.
