The galaxy presents as a highly inclined, disk-dominated system. The central bulge appears to be relatively small and indistinct. A distinct dust lane is not readily apparent, but the slight color variations throughout suggest potential obscuration by interstellar dust within the disk. The disk itself exhibits a smooth texture, without obvious spiral arm structures or distinct star-forming regions detectable in this image. The galaxy is elongated along its major axis, hinting at a flattened structure consistent with an edge-on spiral or lenticular galaxy. There is no visible evidence of tidal disturbances or interactions with other galaxies. The system displays a reddish hue overall, potentially indicating an older stellar population with relatively low ongoing star formation.
