The galaxy presents as a spiral galaxy with a moderately sized bulge. The bulge appears yellowish, indicating an older stellar population. Spiral arms are visible but not sharply defined. The arms appear to be somewhat flocculent and extend a noticeable distance from the central bulge. There is a hint of a bar-like structure bisecting the bulge region. The overall color of the galaxy appears to be relatively evenly distributed with an apparent shift to redder color in the bulge region. There is no evidence of ongoing major merging activity. Based on the morphological structure it seems to have moderate star forming activity. The disk is not viewed edge-on.
