The galaxy presents as a spiral type, with a relatively smooth, but discernible disk. There is evidence of spiral arm structure, exhibiting a moderate winding pattern. The disk shows a slight inclination relative to our line of sight, appearing somewhat elongated. A central bulge is visible, although it does not dominate the overall structure; it appears as a moderate size. The colors are indicative of a mix of stellar populations, with bluer regions suggesting ongoing star formation, and yellow/white areas potentially indicating older stellar populations. There are indications of slight disturbances but does not appear to be undergoing a major merger event. A bar structure seems to be present, possibly of weak to moderate strength, bisecting the central region. Dust lanes and patchy star forming regions can be inferred from the irregularities in the light distribution within the arms.