This galaxy exhibits a clear disk-like structure, indicative of a spiral galaxy morphology. The spiral arms are somewhat tightly wound, showing moderate presence with clear evidence of active star formation occurring within them. These regions manifest as patchy areas of increased blue luminosity within the arms. A central bulge dominates the galaxy's core. The brightness is mostly moderate. The bulge is slightly elongated, and is a yellow color. The colors suggest a mix of stellar populations, possibly including relatively older stars towards the central region and younger stars with ongoing star formation in the spiral arms. There are no obvious signs of major mergers or tidal disturbances. The galaxy appears relatively isolated, with no immediate interacting companions visible.
