This galaxy presents as a spiral, observed at an oblique angle. The spiral arms are loosely wound and well-defined, appearing to emanate from a central bulge. The bulge is relatively compact and moderately bright. The galaxy appears to be of intermediate size, with the spiral structure dominating the overall morphology. There is evidence of ongoing star formation within the spiral arms, indicated by regions of enhanced blue color. No significant signs of tidal interactions or major mergers are immediately apparent, though there may be some minor disturbance in the disk. Dust lanes are subtly visible within the arms, contributing to the overall structure.
