The galaxy exhibits a distinct spiral structure with prominent, well-defined arms extending from a central bulge. The spiral arms appear tightly wound, suggesting a grand design spiral galaxy type. The galaxy is slightly inclined relative to our line of sight. The central bulge appears moderately sized in relation to the overall galaxy disc, exhibiting a yellow-white hue. The spiral arms display bluer colors, indicating regions of active star formation. Dark dust lanes are visible within the spiral arms, obscuring the light from stars behind them. The galaxy is relatively isolated, showing no obvious signs of tidal disturbances or interactions with neighboring galaxies, indicating a relatively undisturbed morphology. There may be a weak bar at the center of the galaxy.