The galaxy presents as a centrally concentrated, luminous object with a largely smooth morphology. Its overall shape approximates a slightly elliptical spheroid, with the major and minor axes appearing nearly equal. There is no obvious spiral arm structure or bar feature visible. The color gradient suggests a possible redder core, though this could also be due to light scattering or dust obscuration. Visual inspection does not reveal any signs of recent major mergers or tidal disturbances. The galaxy's relatively homogeneous light distribution indicates a likely evolved stellar population, consistent with a minimal rate of active star formation.
