This galaxy presents as a spiral galaxy, viewed at a moderate inclination, not quite edge-on. The central bulge is relatively small. Two distinct spiral arms can be identified. There is a prominent bar structure visible across the central region, appearing quite strong. Star formation is present within the spiral arms, indicated by bluer regions. The color of the bulge appears yellowish/white, suggesting an older stellar population. There is no obvious visual evidence of any major merger activity. There is a slight disturbance, indicating a possible minor merger. The galaxy has a moderate amount of rotational symmetry.
