The galaxy presents a disk-like structure, positioned at a moderate angle relative to our line of sight.  Spiral arms are clearly visible. The spiral arms are relatively tightly wound near the center, gradually becoming looser as they extend outwards. It appears as though there are two dominant spiral arms. The central bulge seems relatively small. The galaxy shows a color gradient, with the central region displaying a yellowish hue, suggestive of an older stellar population.  The spiral arms exhibit a bluer tint, indicating the presence of younger, hotter stars and ongoing star formation. There is no apparent major disturbance in the structure to suggest a recent major merger event. Faint dust lanes may be present along the spiral arms, though the image resolution is insufficient for clear identification. A faint bar might be present across the nucleus.
