The galaxy presents an elongated morphology, suggestive of a disk galaxy viewed nearly edge-on. A distinct central bulge is not readily apparent. There are two prominent bright regions; these may be areas of higher stellar density within the disk. There is a slight hint of curvature in the disk's structure, which could indicate the presence of spiral arms or tidal distortions. The colour appears to be dominated by redder wavelengths. There are no obvious signs of recent major merger activity, but the distorted morphology suggests a minor interaction or internal instability.
