The galaxy presents as an edge-on spiral system. A prominent central bulge appears to dominate the light profile, exhibiting a yellowish-orange hue, suggesting an older stellar population. The disk is viewed nearly edge-on, exhibiting a relatively high degree of symmetry. There is a slight indication of warping or tidal disturbance at the extreme edges of the disc. No distinct spiral arm structures are discernable. The color gradient in the disc suggests the presence of dust lanes, though the image resolution limits a precise identification. The galaxy displays a significant amount of internal extinction, impacting the apparent blueness of the disk. Based on its overall morphology, the galaxy does not display obvious signs of a recent major merger event.
