The galaxy presents a clear disk-like structure, viewed at a near edge-on orientation relative to our line of sight. A central bulge is visible, appearing somewhat elongated along the major axis of the disk. The disk exhibits a degree of patchiness, potentially indicative of dust lanes or regions of active star formation within the spiral arms, though these are not clearly resolved. The galaxy shows a smooth profile, with an overall shape showing signs of possible disturbance, but nothing major. The galaxy appears to be relatively isolated, with no obvious signs of interaction with other galaxies. The light is more concentrated in the middle with light stretching out along its edges.
