The galaxy presents as a face-on spiral galaxy with a visible disk structure. The spiral arms are moderately wound, exhibiting both areas of defined structure and regions of more diffuse star formation. Color variation suggests the presence of both older stellar populations and ongoing star formation within the arms. The central bulge is present but not dominant, it appears more as a gradual increase in stellar density toward the center. There is a suggestion of a bar structure across the center of the galaxy. Evidence of tidal disturbances or a potential merger event is present as distorted arm shapes. The overall luminosity is suggestive of a relatively low-mass galaxy with a moderate rate of star formation.
