The galaxy presents as a spiral type, with a prominent disk structure. Two tightly wound spiral arms are clearly discernible emanating from the central region. A moderate bulge is observed at the galaxy's core. A weak bar structure seems to be present across the central region. No significant tidal distortions or indications of ongoing major merger events are apparent. There are some minor disturbances or irregularities observed in the spiral arms, but the overall structure is well-defined. The colour suggests a mix of stellar populations with star formation activity.
