The galaxy presents as a spiral, viewed at a near edge-on inclination. There is a prominent central bulge exhibiting a yellowish hue, suggesting a population of older stars. Extending outwards from the bulge are faint, diffuse spiral arms. The dust lanes associated with the spiral arms are barely discernible but inferred based on the slight variations in color and brightness. The galaxy's overall shape appears elongated, with the major axis significantly longer than the minor axis. There is no apparent evidence of significant tidal disturbances or recent merger activity, although faint asymmetries in the outer disk cannot be ruled out. The galaxy's structure suggests a relatively evolved system.