The galaxy presents as a spiral galaxy with a notable bar structure. The spiral arms are tightly wound around a moderately sized bulge, displaying a distinct two-arm morphology. The galaxy exhibits a blue hue in the outer regions of its spiral arms, potentially indicative of ongoing star formation. A substantial bar spans a significant portion of the galaxy's diameter. There is no evidence of major mergers or significant disturbances, but the galaxy might have had a minor interaction in the past. The disk is viewed at an angle that is not edge-on, allowing for clear observation of the spiral structure.
