The galaxy presents as a moderately bright, elliptical system at a redshift of approximately 0.08. It exhibits a smooth, somewhat spheroidal morphology with a high degree of central concentration. The core region is noticeably brighter and appears slightly elongated. The isophotes are generally smooth, suggesting a well-mixed stellar population with minimal evidence of spiral arms or significant dust lanes. There are no apparent signs of recent major merger events, though minor disturbances cannot be ruled out based on the image alone. The galaxy's color profile indicates a predominantly older stellar population, with a likely lower rate of active star formation. Overall, it is consistent with a relatively quiescent elliptical galaxy residing at an approximate distance.
