The galaxy presents as a relatively smooth, elliptical morphology, although there is a slight elongation. The main body displays a concentrated central bulge that emanates light, indicative of a high concentration of stars. This central region appears to have a yellowish-white hue, possibly suggesting an older stellar population. A fainter, redder component is observed extending below the center of the core, which may be indicative of regions with ongoing or recent star formation. There is no distinct spiral structure visible, which supports a smooth classification. Faint hints of disturbance are present, which could be caused by a past interaction with another galaxy.
