The galaxy appears to be an elongated, disk-like structure, exhibiting a morphology consistent with a spiral or lenticular galaxy viewed at a significant inclination. The central region presents a bright, concentrated bulge, suggesting a substantial stellar population. The light distribution appears smoother than that of a classic spiral galaxy, hinting it could be an older system. Faint spiral arms might be present, but are not well defined. Colors range from blue to red. There is no evidence of a recent major merger, or any other large scale disturbance, although this could use further examination. Overall, the object is not very bright, suggesting that we are seeing it at quite a distance.
