The observed galaxy presents a distinct spiral morphology. The spiral arms are well-defined and exhibit a multi-armed structure. The arms display a moderately tightly wound configuration. The central bulge appears relatively small compared to the disk, suggesting a later Hubble type. The overall color is consistent with ongoing star formation activity, evidenced by the presence of bluer regions within the spiral arms. No significant signs of a major merger event are apparent, although there are slight morphological disturbances which could be signs of an ongoing minor merger, or internal instabilities. A weak bar structure might be present in the central region. The galaxy is not observed edge-on.
