The galaxy presents a generally smooth morphology, appearing largely elliptical in shape with a high degree of roundness. The central region exhibits a bright, concentrated core of light, which diminishes gradually towards the outer edges. Subtle color gradients are discernible, with a bluer hue towards the center possibly indicating the presence of younger stellar populations, and a tendency towards redder tones in the outskirts, suggesting older stars. No distinct spiral arms or prominent dust lanes are observed. There might be a very faint, diffuse halo surrounding the main body of the galaxy, but this is hard to make out given the image. There are no signs of ongoing major mergers or significant tidal disturbances. Overall, the galaxy appears relatively undisturbed.
