The galaxy exhibits a clear disk structure with observable spiral arms. While moderately inclined relative to our line of sight, the disk is not fully edge-on. The central bulge is of moderate size, neither dominating the disk nor appearing insignificant. There may be a faint bar feature present, and the arm structure appears somewhat flocculent. There are hints of potential tidal features or asymmetries, suggestive of a possible past interaction or merger event. The light distribution is clumpy and there appears to be some amount of ongoing star formation. Overall, the morphology suggests an actively evolving spiral galaxy.