The galaxy presents as a face-on spiral, exhibiting a notable degree of symmetry. The spiral arms appear well-defined yet somewhat flocculent, displaying a patchy distribution of light indicative of active star formation regions. The arms emanate from a central bulge that displays a smooth, yellowish profile. There appears to be a weak bar feature extending through the bulge. The bluer hues observed within the arms suggest a relatively high concentration of young, massive stars. Overall the galaxy seems to show no major disturbances or evidence of recent mergers, although there are a few minor irregularities in the spiral arm structure.
