The galaxy presents as a spiral galaxy with a moderately inclined disk relative to our line of sight. The central bulge is prominent, exhibiting a yellowish hue, suggesting an older stellar population. Spiral arms are clearly visible, tracing a somewhat tightly wound morphology. Blue regions indicative of ongoing star formation are observed along the spiral arms, particularly in the outer regions of the galaxy. The dust lanes appear somewhat patchy and irregular, suggesting minor disturbances or tidal interactions, though the overall structure of the galaxy appears largely undisturbed.
