The galaxy appears to be a spiral galaxy, presented roughly face-on with a redshift of approximately 0.022. Evidence of spiral arms can be seen, though they are not sharply defined, indicating a flocculent or grand design spiral structure. There is a central bulge present, though it is not dominant, suggesting a classification of type Sb or Sc in the Hubble sequence. The presence of a bar is suspected, with possibly a weak structure extending from the central region.

The color distribution shows some variation, with bluer regions primarily in the spiral arms, suggesting ongoing star formation. The overall color index, derived from the g, r, and z bands, indicates a relatively blue galaxy, consistent with moderate to low star formation activity. The galaxy does not appear to be significantly disturbed or undergoing a major merger, but there may be evidence of minor tidal features or interactions that could suggest past mergers. The galaxy is relatively compact.
