This galaxy presents as a spiral system with distinct, well-defined arms. The arms display a range of winding tightness, with some regions appearing more tightly wound than others. A central bar structure appears to be present, running through the bulge of the galaxy, with an intermediate strength of stellar density compared to the rest of the disk. The bulge itself seems relatively small compared to the overall disk size. The color distribution suggests active star formation within the spiral arms, indicated by the blue hues and bright spots. There are hints of disturbances in the outer regions of the disk, possibly indicative of past interactions or ongoing minor mergers. The arms appear somewhat flocculent, with multiple arm segments and spurs rather than continuous, grand-design structures. The overall morphology suggests a galaxy that has undergone some degree of interaction or internal activity.
