This galaxy appears to be a spiral galaxy, seen at a high inclination. It exhibits a smooth, elongated structure with a bright central bulge. The disk component is visible, with an indication of spiral arms, though the resolution makes it difficult to discern any distinct features. The color gradient suggests active star formation regions, particularly towards one end of the major axis where a blue hue is observed, and a population of older stars dominates the center. There does not appear to be a very clear dust lane, but some level of obscuration is expected. The morphology is largely undisturbed, with no signs of major interactions or mergers.
