The galaxy exhibits a distinct spiral structure. The spiral arms are prominent and appear loosely wound. Two main arms are discernible, originating from a central bulge region. The bulge is relatively small and compact, with a yellowish hue indicative of an older stellar population. The arms display a bluer color, suggesting ongoing star formation activity. There is no obvious bar structure evident, and there is no clear evidence of a major merger event, however there are some indications of minor gravitational disturbance with small tidal features. The galaxy is viewed at an angle, neither face-on nor edge-on. The overall impression is that of a relatively normal spiral galaxy with active star formation.
