The galaxy presents as an elliptical form, elongated along a major axis oriented roughly diagonally. The central region exhibits a high surface brightness, appearing almost uniformly luminous. The luminosity fades gradually with increasing radial distance from the core, showing no distinct features such as spiral arms or a prominent disk structure. There is a slight color gradient, transitioning from a bluer central hue to redder hues at the outer edges, indicative of differing stellar populations. Overall, the galaxy appears relatively smooth in texture.
