The galaxy presents as a spiral type with a moderate-sized bulge. The winding of its spiral arms appears to be mostly tight. Indications suggest the presence of spiral arms, although the precise count is difficult to ascertain. The disk appears face-on. No strong bar structure is evident. There appears to be no significant merger activity. Based on the color profile, the galaxy exhibits a blue hue in its spiral arms suggesting a substantial rate of star formation. The center of the galaxy is more yellow, suggesting older stars.