The galaxy is a spiral type, exhibiting a clearly defined disk structure. The disk presents a complex morphology with prominent spiral arms. The spiral arms appear tightly wound around a central bulge, which is moderately sized and exhibits a yellowish hue indicative of an older stellar population. The arms themselves display a bluer color, suggesting ongoing star formation. Two prominent spiral arms are easily discernible. There is no apparent bar structure. The galaxy is inclined relative to our line of sight, but not viewed perfectly edge-on. No major mergers are visible, there is a slight indication of a minor disturbance in the form of asymmetrical morphology in one of the spiral arms. The estimated size is approximately 8 kpc in radius.
