The galaxy presents as a disk galaxy, viewed at a shallow angle, appearing somewhat elongated in shape. The central region is bright and relatively featureless, suggesting a significant population of older stars and/or dust obscuration within the nucleus. There are hints of spiral arm structure extending from the central bulge, but the arms appear somewhat flocculent. The disk exhibits varying degrees of brightness, potentially indicative of differing stellar densities or dust lane presence. Overall, the galaxy appears relatively isolated and shows no obvious signs of major mergers or tidal interactions. The colors are mostly muted yellows and reds, suggesting evolved stellar populations across the galaxy. There is some blue scattered throughout the galaxy though, indicating small amounts of star formation are happening. The galaxy doesn't appear to be particularly active.
