The galaxy presents as an edge-on spiral, with a distinct central bulge that appears relatively smooth and concentrated. The overall structure suggests a disk galaxy seen nearly along its plane.

The bulge exhibits a yellow-orange hue, indicative of an older stellar population. Faint dust lanes are subtly visible within the disk, particularly near the central bulge region, suggesting ongoing or recent star formation. The outer edges of the disk appear somewhat faint and diffuse, displaying a blueish tint that may point to a population of younger, hotter stars in the spiral arms. Overall, the galaxy appears undisturbed, with no apparent signs of major mergers or strong tidal interactions.
