This galaxy exhibits a distinct spiral structure, appearing face-on. Prominent spiral arms emanate from a central bulge, although the bulge itself is not dominant in size and the majority of the light of the galaxy appears to come from these arms. These arms appear somewhat tightly wound and exhibit a granular texture, suggestive of ongoing star formation regions. The galactic disc is well-defined. The galaxy displays a prominent bar feature running through its central region. There is no obvious evidence of strong tidal disturbances or major mergers, though subtle irregularities might suggest minor interactions or past disturbances. The color profile indicates relatively active star formation within the spiral arms, but is difficult to discern given the quality of the image.
