The galaxy presents a distinct spiral structure, characterized by well-defined arms that extend outwards from a prominent central bulge. These arms show a consistent pattern, suggesting two main arms. The arms exhibit a medium degree of winding, neither tightly coiled nor loosely extended. The central bulge appears moderately sized, contributing significantly to the galaxy's overall luminosity. A bar structure bisects the central bulge. The image shows signs of a smooth disk in the outer regions, though with notable dust lanes interspersed. This suggests ongoing star formation activity. There is no immediate evidence of major interactions or mergers with other galaxies, although there is a minor disturbance.
