The galaxy presents as a relatively faint, edge-on spiral, characterized by a smooth but discernible disk structure. It exhibits a central bulge that appears slightly brighter than the rest of the disk. The disk is notably elongated, suggesting a high degree of inclination relative to our line of sight. Faint, diffuse spiral arms are implied, but not distinctly visible, perhaps due to the edge-on orientation. The overall color of the galaxy is blue, indicating a moderate level of ongoing star formation. There is a possible indication of minor asymmetry or disturbance in the disk, hinting at a past or ongoing interaction, but no major merging event.
