The galaxy presents as a flattened, disk-shaped structure viewed edge-on. A prominent central bulge is visible, exhibiting a smooth and concentrated distribution of light. The bulge appears to dominate the galaxy's luminosity, suggesting a significant population of older stars. Dust lanes are not clearly discernible within the disk, which may indicate a lack of significant ongoing star formation or obscuration in the regions. There does not appear to be any prominent star formation regions in this image. No evidence of a spiral arm structure is visible, again due to the edge-on orientation. The disk has a noticeable asymmetry. The galaxy appears relatively isolated with no signs of tidal disturbances or ongoing interactions with neighboring galaxies.
