The galaxy presents an elongated morphology, appearing as a somewhat distorted disk viewed at an oblique angle. A brighter, yellowish central bulge is discernible, indicating a concentration of older stars. The disk component exhibits a more diffuse, bluish hue at the edges, suggesting the presence of younger stellar populations and ongoing star formation, although at a relatively low rate. There's a non-uniformity within the disk, potentially indicative of a minor gravitational interaction or disturbance. The galaxy's overall structure is not perfectly smooth, showing some irregularities that suggest it is not a fully relaxed system. It appears to be undergoing a merger, however further investigation is required to determine the severity of this event.
