The galaxy presents as a spiral with a clearly defined disk structure. The spiral arms are prominent, demonstrating a relatively tightly wound morphology. A central bulge is noticeable, with what looks like a moderate presence. The galaxy's overall color suggests a mix of stellar populations, with bluer regions potentially indicating ongoing star formation and redder areas hinting at older stellar populations. There is no obvious indication of a strong bar structure. There may be minor disturbances in the disk, but further investigation is required. The disk is face-on to our line of sight.
