The galaxy presents as an edge-on spiral, exhibiting a notably elongated profile. A prominent central bulge displays a yellowish hue, suggesting an older stellar population concentrated in the core. The disk appears thin and flattened, with a faint bluish tint towards the outer regions, hinting at ongoing star formation within spiral arms that are not clearly resolved due to the edge-on orientation. There is no apparent disruption indicating a major merger, although there may be a slight asymmetry suggesting minor interactions. The bulge shows hints of being rounded. Overall, the galaxy appears as a relatively undisturbed system.
