The galaxy presents as an elongated, edge-on spiral system. A prominent central bulge dominates the overall luminosity profile, exhibiting a smooth, concentrated glow. The disk component, while thin, extends significantly outwards from the bulge, displaying a subtle gradient in luminosity. The dust lane is faintly visible along the equatorial plane, obscuring some of the light from the bulge and disk. The overall color of the galaxy appears relatively uniform, with a slightly redder hue in the central bulge compared to the disk, possibly indicating an older stellar population in the bulge. There is no apparent sign of recent major merger activity or significant tidal disturbances. Faint spiral arm structures are not visible, given the edge-on orientation and resolution.
