The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. The light distribution appears relatively uniform, lacking distinct spiral arms or a prominent bar structure. The core exhibits a yellowish-white hue, potentially indicative of an older stellar population. The outer regions appear somewhat more diffuse with a slight red shift, gradually fading into the background sky. There is no obvious presence of dust lanes or strong tidal features suggesting recent major mergers, however, there are some faint irregularities around the edges, suggesting minor disturbances. Overall, this appears to be a well-formed elliptical galaxy in a relatively quiescent state.
