The galaxy presents as a luminous object with a concentrated central bulge. The overall morphology appears largely smooth, with a hint of a possible disk-like structure oriented in a shallow diagonal line across the image. The central region exhibits a yellowish hue, potentially indicating an older stellar population and/or dust obscuration. The edges of the disk, to the right, are lighter in tone, showing some star formation regions of blues and greens. There is no obvious presence of strong spiral arms, suggesting that it might be undergoing a merger event, where the disk of one galaxy is being disrupted by another. Faint tidal features, or minor disturbances are suspected, based on the distortion of the primary galaxy's shape. There is some evidence suggesting a merger or interaction with a companion galaxy. This could explain its current form and ongoing star formation, as these disturbances can trigger periods of high activity.
