The galaxy presents as a spiral galaxy with a moderately inclined disk. Spiral arms are apparent, exhibiting a somewhat patchy distribution of light, indicating active or recent star formation regions within the arms. There is evidence of tidal disturbances, possibly indicating an ongoing or recent merger event. A central bulge is visible, with a small apparent size relative to the overall disk. The galaxy does not appear to be strongly barred. The morphology suggests ongoing interactions are influencing the structure of this galaxy.
