The galaxy presents a disk-like morphology, observed at a significant inclination relative to our line of sight. A central bulge region is apparent, although not prominently dominant within the galaxy's overall structure. The disk exhibits characteristics of a spiral galaxy, with indications of loosely wound spiral arms extending from the central region. These arms appear somewhat fragmented and lack a highly defined, continuous structure. There is a suggestion of the presence of a bar feature traversing the central region. The overall color of the galaxy leans towards blue, implying ongoing star formation activity, particularly within the spiral arms. The observed light distribution indicates a relatively smooth profile, without any signs of major disturbances from recent mergers. The galaxy shows some signs of having a faint halo.
