The galaxy presents as an elliptical morphology, appearing largely smooth and featureless. The central region exhibits a high concentration of light, which gradually decreases towards the outer edges. There is a slight elongation, but it appears largely circular. No distinct spiral arms or prominent dust lanes are observed. The color profile suggests an older stellar population, exhibiting a reddish-yellow hue. There are no signs of ongoing major merging activity, though some minor disturbances may be present.