The galaxy presents as a somewhat symmetrical, elliptical form. Its core region appears bright and centrally concentrated. The light appears to uniformly decrease in intensity as you move outwards from the center, lacking distinct spiral arms. The central luminosity suggests a high concentration of stars in the core, potentially indicating the presence of a supermassive black hole. The color is generally uniform with only a slight blue tint on the edges. There are no signs of active galactic nuclei activity visible. It also appears as though there might be a small interaction with a smaller galaxy that has a red hue, though it seems to have a small impact on the morphology of the main galaxy.
