The galaxy presents a discernible disk structure. Faint spiral arms are suggested, though not sharply defined. The central bulge appears moderately prominent, exhibiting a yellowish hue, potentially indicating an older stellar population. The disk is generally bluer, suggesting ongoing star formation. There's no obvious indication of a strong bar feature, although there appears to be a slight elongation to the galaxy. No major disturbances or mergers are evident in this image. Overall, the galaxy appears as an average to slightly above average mass spiral galaxy in terms of star formation.
