The galaxy presents a distinct spiral structure, with prominent arms emanating from a central bulge. The arms display a moderate winding pattern. The color distribution suggests a mix of stellar populations within the arms, likely exhibiting active star formation regions interspersed with older stellar clusters. The central bulge appears relatively compact and concentrated. There is no strong visual evidence of a prominent bar structure bisecting the galaxy. The overall morphology indicates a disk-dominated system, with a relatively small bulge in comparison to the disk size. The galaxy exhibits a slight asymmetry in the arm structure, which may hint at a possible gravitational interaction or minor disturbance. There does not seem to be any indications of a major merger event disrupting the structure.
