The observed galaxy presents a distinct spiral morphology. Two prominent spiral arms emanate from a central region. These arms appear tightly wound. A faint bar-like structure can be seen running through the core of the galaxy. The central bulge is not pronounced, appearing relatively small in comparison to the overall disk size. The galaxy exhibits a blue hue, particularly within the spiral arms, suggesting ongoing star formation within those regions. No signs of major mergers or significant tidal disturbances are evident, although a slight asymmetry in the spiral arm structure could indicate a minor interaction in its past.
