The galaxy presents as a lenticular, edge-on system. A central bulge, subtly elliptical, exhibits a yellowish hue, suggestive of an older stellar population. The surrounding disk appears flattened and elongated, with a bluish tint indicative of ongoing or recent star formation within its spiral arms. The dust lanes are not clearly resolved in this image, which is consistent with an Sa or Sb classification. The galaxy displays a smooth light distribution, with no apparent major disturbances or mergers affecting its structure.