The galaxy presents as a somewhat elliptical, disk-like structure with a concentrated, bright central bulge. Its color is predominantly yellow-orange, indicating an older stellar population and reduced star formation. The disk appears smooth and largely featureless, lacking prominent spiral arms or dust lanes. There is a subtle color gradient, with the outer regions of the disk exhibiting a slightly bluer hue compared to the core, suggesting the presence of some younger stars further from the center. No signs of any major mergers or significant tidal disturbances are observed. Overall, the galaxy appears relatively undisturbed and evolving passively.
