The galaxy presents as a relatively smooth, rounded structure. There is a concentration of light towards the center, suggesting a bulge or a core region. The outer regions appear to gradually fade in intensity, indicating a decreasing stellar density with radial distance. A slight color gradient is observed, transitioning from a faint yellow at the center to a slightly bluer hue in the outer regions, which could indicate the presence of younger stellar populations there. No prominent spiral arm structures or significant dust lanes are discernible. Overall, the galaxy appears largely undisturbed, with no signs of major mergers or tidal disruptions visible in this image.
