The galaxy presents a distinct, elongated morphology, viewed at an oblique angle relative to its primary plane. A central bulge region is evident, exhibiting a high degree of luminosity. Emanating from the bulge, spiral arm structures are observed, though their definition appears somewhat diffuse, especially in the outer regions of the galactic disk. These arms possess noticeable substructure, hinting at the presence of star-forming regions. The galactic disk exhibits a complex color gradient, with bluer hues dominating the outer arms and a shift towards redder tones in the inner regions, potentially indicating variations in stellar populations or dust content. Overall, the galaxy appears as a well-formed spiral with a prominent central component and moderately defined spiral arms.
