The galaxy presents as a centrally concentrated, elliptical-like structure. Its overall color is yellowish-orange, suggesting a population of older stars. The light profile appears relatively smooth, with no prominent spiral arms or distinct features visible. A slight elongation is observed, indicating it is not perfectly spherical. The galaxy is relatively compact, exhibiting a high degree of central concentration of light, suggesting a significant bulge component. No obvious signs of recent or ongoing major mergers are apparent, although subtle irregularities in the outer regions might indicate past minor interactions. There may be a limited amount of low-level star formation, based on the slight bluer tinge in some regions, but it is likely dominated by an older stellar population.
