The galaxy presents as a centrally concentrated, elliptical-like structure with a smooth overall appearance. There is a pronounced bulge that appears to be nearly spherical, dominating the galaxy's light profile. The disk component is subtly visible with some flattening, but is not a clearly defined spiral. Overall, it exhibits a moderate inclination relative to our line of sight. It is a substantial galaxy in size, exhibiting redder colors typical of older stellar populations, with weak to moderate levels of ongoing star formation. The galaxy appears relatively undisturbed morphologically, showing no major signs of recent or ongoing mergers.
