The galaxy presents a somewhat edge-on disk morphology. A prominent central bulge dominates the structure, exhibiting a smooth, concentrated luminosity profile with an elliptical shape. The disk component appears elongated and relatively thin, extending outwards from the central bulge. Dust lanes are not clearly visible, but the disk appears partially obscured. The light distribution suggests that the bulge is dominated by older stellar populations, exhibiting a redder hue, while the outer regions of the disk show slightly bluer colors, possibly indicating the presence of younger, hotter stars. Overall the galaxy shows no major signs of recent merger activity or tidal disturbances.