Observed galaxy exhibits a disk-like morphology, presenting as a highly inclined, nearly edge-on spiral. The central bulge is bright and concentrated, appearing somewhat elongated along the major axis. The disk component is visible as a flattened structure extending outwards from the bulge on either side. There is a slight warp or asymmetry visible in the disk structure.

Evidence of possible disturbances is present, indicated by faint tidal features or irregular structures extending away from the main galactic body. These features are relatively subtle, suggesting a minor interaction or past merger event.

Color gradients are visible, with the central bulge exhibiting a slightly redder hue, which could imply an older stellar population, whereas the outer disk displays a bluer tint, possibly indicative of ongoing star formation. There appears to be some degree of patchiness within the disk, suggesting areas of differing stellar density or dust obscuration.
