The galaxy presents as a spiral type, exhibiting a prominent, albeit somewhat ill-defined, disk structure. The spiral arms are readily apparent, with a multi-armed morphology. The arms appear somewhat flocculent, suggesting ongoing or recent star formation. 

The bulge of the galaxy is readily visible and appears to be of moderate size. A bar structure is not clearly visible. The color distribution suggests a population gradient within the galaxy, with the central bulge exhibiting a redder hue compared to the bluer arms. This suggests a relatively older stellar population in the bulge and younger, star-forming regions in the arms.

There is some morphological irregularity, possibly indicating minor disturbances within the galactic structure.
