The galaxy presents as a spiral type, viewed at a slight angle relative to face-on. A central bulge is clearly visible, appearing moderately prominent and exhibits a yellowish hue, suggesting an older stellar population. Faint spiral arms extend from the central bulge. The disk exhibits a bluish tint, indicative of ongoing star formation. There is no apparent strong bar structure visible. The overall structure appears relatively undisturbed, with no obvious signs of major merger activity. There appears to be little dust absorption visible.
