This galaxy presents as a relatively smooth, disk-shaped system seen at a high inclination angle, nearly edge-on from our line of sight. There is a prominent central bulge, which appears to be a yellowish hue, suggesting an older stellar population. The disk extends outward from the bulge, gradually fading in brightness and appearing bluer towards the outer edges, possibly indicating ongoing star formation within the spiral arms. Faint dust lanes are suspected along the disk plane, though the resolution does not permit a definitive identification. The overall structure suggests a spiral galaxy morphology, likely with tightly wound arms. There's a slight asymmetry to the galaxy's shape; the disk appears somewhat warped on one side. No significant tidal features or signs of a major merger are discernible, although some subtle disturbances could be present in the outer disk. The light distribution is relatively concentrated, indicating a mature system that has been evolving for a considerable period of time.
