The galaxy presents a distinct spiral morphology. The nucleus appears bright and somewhat diffuse, suggesting the presence of a central bulge. Faint spiral arms emanate from the core region. The spiral arms display a relatively tight winding pattern around the central bulge. The color gradient indicates ongoing star formation within the arms. There are several patches of light spread around the galaxy, these could potentially be areas of concentrated star formation or areas of mass that is lumpy in nature. Overall, the galaxy appears to be relatively undisturbed, with no major signs of recent merger activity. The galaxy appears to be relatively face on to our view. A slight bar may be present.
