The galaxy appears as a centrally concentrated, relatively smooth structure. Its morphology suggests characteristics somewhere between a lenticular and an elliptical galaxy. The galaxy exhibits a slight elongation, but it is predominantly rounded in shape. The color profile is generally consistent, with a central yellowish hue that gradually fades towards the outer edges. There is no discernible evidence of prominent spiral arms or active star formation regions. Faint disturbances are present, but the object shows little evidence of recent or ongoing major merging activity.
