The galaxy presents as an elongated, edge-on spiral or lenticular galaxy with a prominent central bulge. The bulge exhibits a smooth, centrally concentrated luminosity profile suggesting a well-formed spheroid, likely dominated by older stellar populations. The disk appears relatively thin and exhibits a faint, diffuse bluish tint, possibly indicating the presence of some ongoing, albeit low, star formation. Dust lanes may be present along the galactic plane, though these are not sharply defined, contributing to the galaxy's smooth appearance. No signs of major tidal disturbances or recent merger activity are discernible. The overall color index suggests a mature galaxy with an intermediate population of stars. The galaxy’s morphology is consistent with a high degree of disk inclination, with a possibly boxy or rounded bulge.