The object presents as an elongated, disk-like galaxy, viewed edge-on. It exhibits a smooth overall appearance, with no readily discernible spiral arm structures or distinct star-forming regions in this imaging. The central bulge appears prominent and somewhat brighter than the rest of the disk. Color gradients suggest potential stellar population differences across the galaxy, where the central region appears to be redder, suggesting an older stellar population, while the outer regions show a slight blue tint possibly indicating some ongoing star formation. The galaxy displays a high degree of oblateness. There is no obvious sign of a strong interaction or major merger events occurring with other galaxies or structures based on the smooth form of the galaxy. Slight dust lane structures could be present, though the image resolution makes it difficult to confirm.
