The galaxy presents as an elongated, disk-like structure with a clearly defined central bulge. The bulge exhibits a smooth, concentrated brightness, suggesting an older stellar population. Surrounding the bulge, the disk appears relatively thin and exhibits a subtle color gradient, transitioning from a slightly bluer hue in the outer regions to a more yellowish tint closer to the bulge. This color variation implies ongoing or recent star formation in the outer disk regions. A subtle dust lane is observed near the bulge, slightly obscuring the light. The galaxy appears relatively undisturbed, showing no signs of major mergers or tidal interactions.