The galaxy presents as a relatively smooth, elliptical-like structure, exhibiting a high degree of central concentration. The light distribution appears to be consistent with an older stellar population, with a dominant reddish-yellow hue, indicative of a dearth of ongoing star formation. There is a lack of any prominent disk-like features or spiral arms. The overall shape is generally round. There is no obvious indication of any major disturbances or ongoing merger activity. 
