The galaxy exhibits a clear spiral structure, viewed at an oblique angle. Its disk is prominently featured, showing discernible spiral arms. The arms appear somewhat tightly wound near the central bulge, transitioning to a medium winding further out, implying differential rotation. 

The bulge component constitutes a substantial portion of the galaxy's overall luminosity. Within the bulge, there is a bar-like feature. The central region exhibits a smooth, concentrated light profile indicative of an older stellar population.

There's evidence of ongoing or recent star formation within the spiral arms, indicated by the bluer hues and patchy distribution of light. The dust lanes are visible within the arms, particularly on the near side, suggesting obscuration of background starlight. Overall, the galaxy shows no major signs of morphological disturbance.
