The galaxy presents as a face-on spiral with a prominent central bulge. The bulge appears yellow-white, suggesting a significant population of older stars. Two distinct spiral arms emanate from the central region and wrap around the galaxy, exhibiting a medium winding pattern. The arms display a blue hue, indicative of ongoing star formation activity. There is no evidence of significant morphological disturbance to suggest a major ongoing or recent merger event, however, there is some asymmetry visible. A subtle bar-like structure may exist within the central region, and a moderate bulge is apparent. The arms are fairly open and defined.
