The galaxy displays a prominent, well-defined spiral structure. Two distinct arms emanate from a central bulge region, appearing tightly wound closer to the core and gradually loosening as they extend outward. The bulge is moderately sized, exhibiting a yellowish hue that possibly indicates an older stellar population. Patchy regions within the spiral arms showcase a bluer color, suggestive of ongoing star formation. The disk appears relatively undisturbed, showing no visible signs of a major merger event, although minor disturbances cannot be ruled out at this resolution. There's a faint suggestion of a bar-like structure spanning the core region. The galaxy presents a predominantly face-on orientation, allowing for a relatively clear view of its spiral morphology.
