The galaxy presents as a grand design spiral, viewed approximately face-on. Two prominent spiral arms emerge from the central bulge and are tightly wound. A moderate central bulge is visible, its light yellow, indicating an older stellar population. The spiral arms exhibit a bluer hue, suggesting regions of ongoing star formation. The galaxy shows no sign of any major disturbance or merging with another galaxy. A faint, possibly broken, bar structure may be present across the center of the disk. The galaxy is somewhat compact in size.