The galaxy presents as an elongated, edge-on spiral or lenticular galaxy. A central bulge is apparent, displaying a yellowish hue, suggesting a population of older stars. The disk component appears relatively thin and faint, with subtle indications of dust lanes running along the plane of the galaxy. These dust lanes are visible as darker regions within the bluish light of the disk, especially near the periphery. The outer regions of the disk are faint and blurred, making it difficult to resolve individual features, although subtle clumping of light suggests spiral arm structure. There is no obvious evidence of significant tidal distortions or major ongoing mergers. The overall impression is of a galaxy with a well-defined bulge and a quiescent disk.
