The galaxy presents a well-defined spiral structure. Two prominent spiral arms emanate from a central bulge. The spiral arms are characterized by a somewhat flocculent morphology, displaying regions of concentrated star formation interspersed with less dense areas. These regions of higher density exhibit a bluer hue, suggesting the presence of younger stellar populations.

The central bulge appears moderately prominent, displaying a yellowish-orange color, indicative of an older stellar population and potentially a higher concentration of dust. The galaxy does not exhibit obvious signs of a strong bar structure; however, a subtle elongation might be present across the central region. The galaxy appears relatively isolated, showing no clear evidence of a major ongoing merger event, but there is a very minor amount of disturbance in the disk. The overall winding of the spiral arms seems relatively consistent with an intermediate type, neither tightly wound nor completely open. The galaxy is viewed at a moderate angle, allowing for a clear visualization of the spiral arm structure without being edge-on.
