The galaxy presents as an elongated, edge-on spiral galaxy with a faint disk. There is a prominent central bulge, which appears smooth, rounded, and gradually fades into the disk. The disk appears relatively thin. There is no visible spiral arm structure or dust lanes from this angle. The overall color is bluish-white, suggesting the presence of intermediate to old stellar populations. There are no signs of merging or tidal disturbances observed in this image. The light distribution indicates a centrally concentrated mass profile, with a relatively high Sersic index. The lack of significant blue color in the disk suggests low levels of current star formation.
