This galaxy presents a distinct spiral structure. Its morphology indicates a prominent disk, exhibiting well-defined spiral arms. These arms appear tightly wound and extend from a noticeable central bulge. The bulge seems moderate in size relative to the overall galactic disk.

There is a subtle color gradient, with the central bulge displaying a yellowish hue, possibly indicating an older stellar population. The spiral arms, in contrast, show a bluish tint, suggestive of the presence of younger, hotter stars and active star formation. Some arm irregularities may be present, and they suggest minor disturbances.