The galaxy appears to be a spiral galaxy, viewed nearly edge-on, presenting a flattened, elongated shape. The central bulge is prominent and displays a yellowish-white hue, indicating a population of older stars. Moving outward from the core, the disk exhibits a bluer color, suggesting the presence of younger stellar populations and ongoing star formation, though not at a high rate. Some areas appear mottled, and may show some disruption, perhaps indicating a minor interaction. The overall structure suggests a system that is largely settled.
