The galaxy presents as an elongated, spindle-like structure, strongly suggestive of an edge-on or nearly edge-on spiral galaxy. A bulge is visible, appearing centrally concentrated and exhibiting a yellowish-white color, indicative of an older stellar population. Extending outward from the bulge, the galactic disk is noticeably flattened, displaying a bluish hue along its edges. This blue coloration likely signifies regions of ongoing star formation. There is an area of red, likely gas, near one end. The overall smoothness of the light distribution across the galaxy indicates a relatively undisturbed morphology, with no obvious signs of major mergers or tidal distortions.
