The galaxy presents a flattened, disk-like morphology, suggesting it may be a spiral or lenticular type. It is observed at an oblique angle, but significantly inclined, nearly edge-on, relative to our line of sight. A bulge component is visible, appearing as a concentrated region of light towards the center of the galaxy; the bulge appears yellowish in color. The galactic disk exhibits a smooth appearance, with indications of subtle structure that could be spiral arms or dust lanes, but these features are faint. The outer regions of the disk seem to fade gradually into the background, lacking sharp boundaries. The color profile suggests a population of older stars residing in the bulge.
