The galaxy appears to be a relatively smooth, elliptical galaxy, exhibiting a high degree of central concentration. The galaxy's core region displays a yellowish-orange hue, suggestive of an older stellar population dominated by redder stars. There is a slight elongation or deviation from perfect circularity, hinting at a possible cigar shape. The presence of a second, smaller, fainter component slightly offset from the main body may indicate a minor disturbance or potential interaction event. The overall morphology suggests it has likely undergone a relatively quiescent evolutionary history, with little evidence of active star formation.
