The galaxy presents a face-on orientation relative to our line of sight, revealing a clear disk structure. Spiral arms are evident, exhibiting a relatively tight winding pattern. The bulge appears to be of moderate size relative to the overall disk. There is no indication of a strong central bar. The disk shows some flocculent structure, and blue knots are distributed throughout the arms, indicative of star forming regions. While the overall structure appears generally undisturbed, there may be some minor interactions at play, as evidenced by slight asymmetry in the arm structure. 
