The galaxy presents as an edge-on spiral, with a prominent bulge and a highly flattened disk. The bulge appears yellowish, suggesting an older stellar population. The disk shows a faint bluish hue, potentially indicating regions of ongoing star formation, though these regions are not clearly resolved. No distinct spiral arm structure is visible given the edge-on orientation. There is some evidence of a slightly boxy shape to the bulge. The galaxy appears relatively undisturbed, with no obvious signs of a recent major merger event.
