The galaxy appears to be a spiral galaxy viewed at a slight angle. There is evidence of spiral arm structure, but the arms are somewhat flocculent and not sharply defined. The color is dominated by blue, particularly in the outer regions of the disk, which suggests a relatively young stellar population and ongoing star formation. The central bulge is present but not particularly prominent, indicating the galaxy may be of later type. There are no obvious signs of a strong bar structure or a significant dust lane. The galaxy appears to have some signs of minor disturbances or irregularities in its overall structure. There may be interactions with nearby objects, or it may be undergoing minor merging events.
