The galaxy appears to be a disk galaxy, likely seen at an oblique angle. It exhibits a smooth, centrally concentrated bulge with a flattened disk. The disk shows a subtle but noticeable asymmetry, possibly indicative of past interactions or internal disturbances. The overall color is bluish, suggesting the presence of a younger stellar population and ongoing star formation. The galaxy appears relatively isolated with no immediately obvious signs of a major merger event, although subtle tidal features might be present upon closer inspection.
