The galaxy presents as an elongated, edge-on spiral. A distinct bulge is not readily apparent, instead there is a central concentration that gently fades to a sharp edge, suggesting a disk galaxy viewed nearly perfectly edge-on. The central region displays a yellowish color, likely indicating an older stellar population. Moving away from the center, the disk shows a subtle transition towards bluer hues, suggesting the presence of younger, hotter stars in these outer regions. Dust lanes are not clearly visible, though there appears to be some mottled obscuration running along the central plane. The overall structure suggests a relatively undisturbed morphology, with no obvious signs of tidal interactions or major mergers.
