The galaxy presents a distinct edge-on morphology, characterized by a flattened disk structure. The central bulge appears prominent and exhibits a rounded profile. Little to no evidence of spiral arm structure is visible, likely due to the edge-on viewing angle. Faint dust lanes are suspected near the mid-plane of the disk, causing a subtle obscuration of starlight. There is no evidence of a recent major merger, however, a possible minor interaction with a smaller companion is suspected due to a slight warp in the disk. The galaxy displays a redder color index compared to typical spiral galaxies, suggesting an older stellar population and reduced current star formation activity. The galaxy appears to be relatively massive.
