The galaxy presents as a disk-shaped structure, viewed at a significant inclination. There appears to be a central bulge, brighter and more concentrated, exhibiting a yellowish hue. The disk itself is relatively smooth in appearance with a greenish color, potentially indicating ongoing star formation. The structure has a well-defined edge. There is no obvious spiral structure, the disk seems relatively featureless. The galaxy does not show any signs of major disturbances that might be indicative of a recent major merger event. The overall color profile indicates a population of intermediate to old stars, mixed with younger, star-forming regions. The morphology could be broadly classified as a lenticular galaxy, but a more detailed analysis of its stellar populations and gas content would be needed for a definitive classification.
