The galaxy presents a distinct spiral morphology. Traces of spiral arms are evident, extending from a central bulge. The bulge itself appears moderately sized, with a smooth, concentrated light distribution, which is characteristic of older stellar populations. The spiral arms are not tightly wound, exhibiting a more open structure. The galaxy’s disk shows a bluer color, indicative of more recent star formation activity. No significant signs of tidal disturbances or ongoing major mergers are visible. However, some irregularities in the spiral arms hint at possible minor interactions or internal disturbances. The galaxy's overall color suggests a mix of stellar populations, with a significant contribution from both older stars in the bulge and younger stars in the disk.
