The galaxy exhibits a disk-like morphology, viewed nearly edge-on. A central bulge is apparent, appearing as a bright, concentrated region with a somewhat rounded shape. Faint, diffuse extensions are visible extending outwards from the central region. These appear to be spiral arms on the far side of the bulge.

Dust lanes may be present within the disk, though the resolution of the image makes it difficult to confirm their presence. The galaxy's color profile appears to be largely in the yellow to red bands, which may imply that the light is composed of older stars with ongoing star formation. Some blue light is visible as well, possibly showing the location of newer star formations.

The disk appears relatively undisturbed, with little sign of major tidal interactions or mergers. Faint irregularities may be present, but the resolution does not allow for definitive identification of any tidal features. Overall, this galaxy appears to be a relatively undisturbed disk galaxy viewed at a high inclination.
