The galaxy appears as an elongated, disk-shaped structure, viewed nearly edge-on. The central bulge exhibits a moderate concentration of light, appearing somewhat rounded. The disk is relatively smooth in texture, showing limited evidence of distinct spiral arm features or prominent dust lanes. There are no obvious signs of a recent major merger event. Based on the colors present, the galaxy shows a mix of older stellar populations, concentrated in the bulge, and younger stellar populations distributed within the disk. The galaxy is relatively faint with a compact structure.
