The galaxy presents a smooth, elliptical morphology with a high degree of central concentration.  The core exhibits a yellowish-gold hue, suggesting an older stellar population dominated by evolved stars.  There is little evidence of spiral arm structure or significant dust lanes.  The galaxy appears highly spheroidal, exhibiting a near-circular shape with minimal elongation. Faint, diffuse emission extends outward from the central region, forming a shallow halo.  There is no clear indication of recent major merger events or significant tidal disturbances within the galaxy's immediate environment. The overall color suggests a relatively quiescent galaxy with a low star formation rate.
