The galaxy presents as an edge-on disk galaxy. There is evidence of a central bulge, with hints of a boxy or peanut-shaped structure. The bulge appears to be surrounded by a faint disk that extends beyond the bulge's immediate vicinity. The disk shows some degree of internal structure, suggesting the presence of dust lanes or spiral arms. Color variations across the galaxy might indicate differences in stellar populations or star formation activity, with bluer regions potentially associated with ongoing star formation and redder regions with older stellar populations. There is no strong evidence for an active galactic nucleus or major merger events, though minor disturbances cannot be ruled out. The overall smoothness of the galaxy suggests that it is a well-established system with no recent major interactions.
