The galaxy presents as a highly inclined, likely late-type spiral system. It exhibits a flattened disk structure with a prominent central bulge. The bulge appears relatively smooth and featureless, exhibiting a yellowish-white color, suggesting an older stellar population. The disk shows evidence of spiral arm structure, though not sharply defined. Hazy blue regions interspersed along the disk are suggestive of on-going star formation. Dust lanes are subtle but appear present, particularly along the near side of the disk, attenuating light and contributing to the galaxy's overall redder appearance. The galaxy has a significant radial extent, indicating a substantial physical size. Its overall morphology appears relatively undisturbed, lacking obvious signs of a major merger or tidal interactions.
