The galaxy presents as a spiral type, observed at an oblique angle. Two prominent spiral arms are clearly visible, loosely wound around the central bulge. The arms appear relatively patchy, suggesting active star formation regions distributed along their lengths. The central bulge is moderately sized, exhibiting a somewhat diffused appearance. There is a possible weak bar feature that extends across the central bulge along its major axis. Overall, the galaxy exhibits a relatively organized structure, without any significant signs of recent major merging activity, though there may be some minor disturbances visible. The color suggests a moderate amount of ongoing star formation activity.
