The galaxy presents as a relatively bright, well-defined elliptical or lenticular system, appearing somewhat flattened. A prominent central bulge dominates the structure, exhibiting a yellowish-orange hue suggesting an older stellar population. Fainter bluish colors are visible in the outer regions indicating younger stars. Overall, the galaxy appears relatively smooth in texture. There is no obvious sign of active galactic nuclei emission or strong dust lane obscuration. There is only a very slight indication of any major disturbances within the galaxy.
