Observed is a galaxy, likely a spiral, seen at an oblique angle. A prominent central bulge is visible, characterized by a yellowish-white hue, suggesting an older stellar population. The bulge constitutes a moderate fraction of the overall galactic structure. Fainter spiral arms extend from the bulge into the galactic disc. The arms appear somewhat diffuse and patchy, indicative of ongoing, but not necessarily vigorous, star formation. The spiral arms also have a bluish hue indicating a younger stellar population. The disc of the galaxy shows signs of slight disturbances, but overall it seems to be unperturbed. There is no presence of a bar structure spanning the central bulge. The system is generally not undergoing any major merging events.
