The galaxy presents as a spiral, viewed at an angle approaching face-on. Several spiral arms, are clearly visible, exhibiting a tightly wound morphology. The spiral arms appear to be grainy, perhaps suggesting areas of ongoing star formation within. The central bulge is of moderate size and appears bright and concentrated, indicating a significant population of older stars. A bar structure is present, of modest strength, traversing through the core of the bulge, indicating this is a barred spiral galaxy. The galaxy does not present evidence of significant morphological disturbance, implying it is not currently undergoing a major merger event. The disk component of the galaxy is more prominent than any smooth and featureless component.
