The galaxy exhibits a generally smooth, elliptical morphology. It presents as a concentrated spheroid of light, brightest at its core, with a noticeable, gradual decrease in luminosity moving outward. The galaxy appears largely undisturbed, lacking strong indications of spiral arms or significant tidal features. A slight elongation is observed, with an axis ratio indicating it is somewhat flattened. Color gradients are subtle, with a redder hue toward the central region that may indicate an older stellar population. The outer regions appear somewhat bluer, potentially suggesting the presence of younger stars. Faint red arm-like features are visible along the edge of the spheroid.