The galaxy exhibits a prominent disk structure with a high probability of spiral arms. It is not viewed edge-on. Two spiral arms are visible, appearing loosely wound. A central bulge of moderate size dominates the inner region. There appears to be a weak bar structure. There is a high likelihood of recent star formation, evidenced by the blue light in the arms. There is no strong evidence of a major merging event; however, there are minor disturbances. Based on the relatively symmetric structure and defined spiral arms, the galaxy is likely in a relatively undisturbed state.
