The galaxy appears to be a spiral galaxy with a disk-like structure. There is evidence of spiral arm structure, though it is not sharply defined. The central bulge is of moderate size, appearing neither dominant nor insignificant within the overall structure. The galaxy displays a prominent blue hue, suggesting a relatively high rate of star formation activity. The overall light distribution indicates a fairly uniform distribution of stars throughout the disk with subtle variations in color and brightness. No strong bar feature is immediately apparent. The galaxy seems relatively isolated, with no major signs of ongoing merger activity.
