This galaxy presents a spiral morphology. The disk is viewed at an angle near edge-on, but not perfectly so. There is a definite central bulge, but it does not dominate the overall structure. It appears to have two well-defined spiral arms. The spiral arms are tightly wound around the galactic center. There's some indication of a possible bar structure crossing the bulge region. The galaxy has a smooth appearance overall, with some areas showing a slight amount of dust or star forming regions. The overall color suggests a mix of older stellar populations. There appears to be no ongoing major merger.
