The galaxy presents a generally smooth and centrally concentrated morphology, with an elliptical appearance. The light is predominantly yellowish-orange, suggesting an older stellar population, with a small amount of more recent star formation. There is a slight elongation, deviating from a perfectly circular form. No obvious spiral arm structures are visible, nor are there any indications of a major merger event, although there is a slight disturbance in the upper right quadrant. The galaxy is relatively compact, occupying a small area in the image, suggesting either intrinsic smallness or great distance.
