The galaxy presents as a relatively smooth, elliptical-like structure. Its overall form is quite round, exhibiting a high degree of symmetry in its light distribution. There is a concentrated central bulge or core. The color is predominantly yellowish-orange, implying an older stellar population. The light tapers off relatively quickly from the core, suggesting a limited presence of extended stellar structures or a faint halo. There appears to be no major disturbances in the shape or notable tidal features, indicating the absence of recent major mergers or interactions. No distinct spiral arm structures or dust lanes are discernible. Overall, the galaxy seems to be an evolved system with little ongoing star formation.
