The galaxy presents an elongated, cigar-shaped morphology. The light distribution suggests a central bulge that appears relatively smooth and concentrated, with a yellowish-orange hue. Fainter and bluer light extends away from the center, indicating a disk structure viewed at a high inclination. There is very little visible structure within the disk suggesting smooth arm features. The overall color suggests that the galaxy is dominated by an older stellar population, with some evidence of ongoing, though limited, star formation. No significant signs of tidal disturbances or ongoing mergers are apparent.
