The galaxy exhibits a clear spiral structure, albeit with tightly wound arms. The arms appear somewhat fragmented and not as distinctly defined as in grand design spirals. There is evidence of ongoing star formation within the spiral arms, indicated by the bluish hues. A moderate bulge component is visible, appearing yellowish in color, which suggests an older stellar population compared to the bluer star-forming regions. The galaxy is viewed at an angle where the disk isn't fully face-on but is not quite edge-on either. There are potential signs of a minor disturbance in the morphology, possibly due to a past interaction, though no clear merger is occurring at the present time based on this image. Overall, this galaxy presents as a spiral with a moderate bulge and active star formation.
