The galaxy exhibits a prominent, well-defined spiral structure. The spiral arms are loosely wound and extend outwards from a central bulge. These arms appear somewhat patchy, suggesting an uneven distribution of star-forming regions. There are visible knots of brighter regions within the arms, indicative of active star formation, and they appear bluer in color.

The central bulge is moderately sized and appears relatively smooth and concentrated, exhibiting a yellowish-orange hue, possibly representing an older stellar population.

There's some indication of a bar-like structure across the center of the galaxy, but it is not particularly strong or well-defined. There are no clear signs of any major mergers or significant tidal disturbances. The galaxy's overall morphology suggests it is a relatively undisturbed spiral galaxy with ongoing, albeit not extremely vigorous, star formation.
