The galaxy presents as a moderately sized, disk-shaped system viewed at a high inclination, approaching edge-on. The central bulge is prominent, appearing as a bright, concentrated region with a yellowish-white hue. The disk exhibits a bluer color, indicating the presence of younger stellar populations and ongoing star formation. There's a subtle irregularity in the disk's structure and faint dust lanes are potentially visible in certain regions. No obvious signs of major mergers are observed; however, minor disturbances within the disk cannot be ruled out. Overall, the galaxy appears as a relatively undisturbed, actively star-forming system.
