The galaxy presents a primarily disk-like morphology, although it is not perfectly face-on. Evidence of spiral arm structure is present but somewhat diffuse. A central bulge is visible, appearing relatively smooth and concentrated. The disk exhibits areas of bluer color, suggestive of ongoing star formation, interspersed with yellower regions possibly populated by older stellar populations. There is a slight indication of a minor disturbance in the galaxy's structure, it is not completely symmetric and may have experienced a minor interaction. Overall, the galaxy appears as a spiral galaxy with signs of recent star formation and a modestly sized bulge.
