The galaxy presents as a moderately luminous, elongated structure. It exhibits a relatively smooth morphology, with a centrally concentrated bulge that gradually fades into a less distinct outer region. The overall color appears relatively red, suggesting an older stellar population with lower levels of recent star formation. There is no clear evidence of spiral arm structure or significant dust lanes. The galaxy's shape is elongated, with a moderate axial ratio, indicating that it is observed at a significant inclination. No signs of recent major merging events or tidal disturbances are apparent, although some minor asymmetry might be present in the outer regions.
