The galaxy presents as a flattened, elongated structure indicative of a disk galaxy viewed at a significant inclination. The central region displays a brighter, more diffuse glow, suggesting a bulge component. The overall color is slightly blue, hinting at the presence of a younger stellar population and ongoing star formation. Some slight disturbances are present, but it is difficult to say if this galaxy is undergoing a merger. The galaxy's structure appears relatively smooth, with no prominent spiral arms immediately discernible in this image.
