The galaxy presents as a flattened elliptical shape, with a visible disk structure. It is oriented at an angle relative to our line of sight. The central region exhibits a higher luminosity than the outer regions, suggesting a concentration of stars and potentially a supermassive black hole at the galactic nucleus. The light is slightly bluer in the central and disk regions. The galaxy appears relatively smooth in texture, without prominent spiral arms or irregular features. This smoothness is most likely due to a relatively low rate of star formation and a more evolved stellar population.
