This galaxy appears to be a spiral galaxy with a well-defined disk structure. There is evidence of tightly wound spiral arms. A strong bar feature is present, bisecting the central bulge. The bulge itself appears to be of moderate size relative to the disk. The spiral arms are relatively symmetrical. There are no obvious signs of a major ongoing merger or significant tidal disturbances. The central bulge exhibits a yellow-white hue, suggesting an older stellar population, while the spiral arms display a bluer color, possibly indicating more recent star formation. There are what may be three or more spiral arms emanating from the bar. The galaxy does not seem to be edge-on.
