The galaxy presents as an edge-on disk galaxy with a prominent central bulge. The bulge region exhibits a concentrated, bright glow, suggesting a high density of stars. The disk component appears relatively smooth, with a noticeable dust lane running along the major axis, bisecting the galaxy. The overall color gradient indicates a redder hue in the bulge and a slightly bluer tint towards the outer disk, possibly suggesting a younger stellar population residing within the disk. No distinct spiral arm structures are clearly visible due to the edge-on orientation, however, there is some evidence of minor disturbances in the disk which could indicate interactions.
