The galaxy presents as a spiral, inclined at a moderate angle to our line of sight. Two prominent spiral arms are clearly discernible. The arms appear tightly wound, displaying a high degree of structure. A notable central bulge dominates the galaxy's morphology. The bulge exhibits a smooth profile and is intermediate in size compared to the overall galactic disk. Evidence of a bar structure is present, extending through a portion of the central region of the galaxy. The dust lanes are somewhat obscured, and the colors are muted and lack distinct bright spots of recent star formation. 
