The galaxy presents as a somewhat flocculent spiral structure. The disk component is readily apparent, displaying a moderate inclination relative to our line of sight. The spiral arms exhibit a patchy distribution of star-forming regions, characterized by a bluer color, indicative of younger stellar populations. These regions are interspersed with areas of relatively less star formation, appearing redder, indicative of older stellar populations. The central bulge region appears relatively smooth and exhibits a more yellowish/reddish hue, suggesting a higher concentration of older, evolved stars. There is no obvious presence of a prominent bar structure. No major merger activity is seen, although there appears to be a slight distortion in one of the spiral arms possibly due to a minor interaction. The overall structure shows a well-defined disk, suggesting it is a relatively settled system.
