The galaxy appears to be a spiral galaxy viewed at an oblique angle, displaying a disk-like structure with discernible spiral arms. The arms exhibit a somewhat patchy morphology. The central bulge is prominent and appears relatively smooth and concentrated compared to the disk. There's evidence of a bar-like structure extending from the central bulge. The color distribution suggests varying stellar populations and dust content across the galaxy; the bulge exhibits a yellowish hue, possibly indicative of older stellar populations, while the disk shows bluer regions potentially associated with ongoing star formation. The galaxy appears to be relatively isolated with no obvious signs of major interactions or mergers. The galaxy is elongated.