The galaxy presents as a somewhat smooth, disk-like structure seen nearly edge-on. A central bulge is not clearly defined in the available image, with the light distribution appearing relatively uniform along the visible plane of the disk. Some subtle features within the disk may suggest minor disturbances or asymmetries. No strong evidence of a recent or ongoing major merger is apparent, though subtle irregularities in the disk's structure warrant further investigation. The color is not strongly indicative of recent star formation, and the light emitted from the galaxy appears redder.
