The galaxy exhibits a clear spiral structure, characterized by prominent arms emanating from a central bulge. These arms are traced by regions of active star formation, indicated by their bluish hue and the presence of numerous bright knots. The spiral arms appear relatively tightly wound, wrapping closely around the galactic nucleus.

The central bulge of the galaxy appears moderately sized, exhibiting a smooth, concentrated distribution of stars. The disk of the galaxy is inclined at a moderate angle to our line of sight, allowing for a clear view of the spiral arm structure.

There are no indications of any major mergers or significant tidal disturbances affecting the overall morphology of the galaxy. It appears to be a relatively isolated system undergoing normal spiral evolution. The galaxy displays a subtle color gradient, with the central bulge appearing more yellow and the spiral arms exhibiting a bluer color due to the presence of younger, hotter stars.
