The observed galaxy presents as a spiral morphology, displaying prominent spiral arms. These arms are loosely wound and exhibit a primarily two-arm structure. A significant portion of the disk is visible, indicating a face-on orientation relative to the observer.

A central bulge is apparent, though it appears relatively small in size compared to the overall galactic disk. There is evidence of a bar structure bisecting the bulge. The bar is of moderate strength, it is clearly defined within the bulge region and extends outwards. The central region exhibits a yellowish hue, likely indicating an older stellar population, while the spiral arms show a bluer color, consistent with ongoing star formation.

There is no visible indication of major galactic mergers or significant disturbances in the overall structure. The galaxy appears to be relatively isolated. The spiral arms exhibit clumpy structures, potentially indicating star-forming regions.
