This galaxy presents as a relatively small, disk-shaped structure seen at a high inclination. The central region exhibits a bright, concentrated core. A surrounding disk-like structure appears prominent, displaying distinct color variations across its extent. A noticeable color gradient is observed from the inner to outer regions, suggesting potential differences in stellar populations or dust content. Specifically, the inner regions appear more yellow, which may indicate older stars or the presence of dust. The outer regions are a pale blue, and seem thinner than the inner regions, possibly indicating younger stellar populations and reduced dust obscuration. Faint irregularities or subtle distortions are visible in the outer regions, possibly indicative of minor gravitational interactions or internal disturbances. There are also a few bright spots within the galaxy which could suggest nebulae. There are no distinct spiral arms are apparent in this image.
