This galaxy exhibits a clear disk structure with evidence of spiral arms, although the resolution limits detailed tracing. The central bulge is prominent and appears moderately sized in relation to the disk. There may be a weak bar feature extending through the galactic center. Dust lanes appear to be present along the spiral arms and within the disk. The galaxy is observed nearly edge-on, its overall shape is flattened, displaying a significant ellipticity. The galaxy color profile suggests a range of stellar populations, with a central yellowish hue possibly indicating older stars in the bulge, and bluer regions potentially outlining younger stars in the spiral arms. There is a hint of a minor disturbance in the shape, suggesting a possible past interaction.
