The galaxy appears to be a spiral galaxy, presenting a near face-on orientation. While the disk component dominates the visual appearance, a moderate central bulge is discernible. Faint spiral arms are present, exhibiting a relatively medium winding, tracing outwards from the central region. The arm structure appears somewhat flocculent. A relatively low fraction of ongoing mergers is visible, with only minor disturbances visible to the overall structure. The galaxy's morphology indicates a classification of a spiral galaxy with an intermediate bulge size and well-defined spiral arms.
