The galaxy presents a clear spiral structure. The arms are well-defined and extend noticeably from the central bulge. The bulge itself is of moderate size, appearing neither overly dominant nor negligible in proportion to the disk. There may be a weak bar feature, but the resolution of the image does not allow definitive confirmation. The galaxy is viewed close to face-on, which enhances the visibility of its spiral arm structure and limits any potential obscuration.

There is color variation across the galaxy. The central bulge shows a yellowish hue, suggestive of an older stellar population. The spiral arms display bluer tints, which likely indicate the presence of younger, hotter stars.
