The galaxy appears as a luminous, elliptical object with a smooth and concentrated light profile. It exhibits a distinct yellowish-red hue, potentially indicative of an older stellar population or significant dust content. There is a noticeable lack of defined spiral arms or a prominent disk structure; it presents as a largely featureless spheroid. The morphology suggests a relatively evolved system with a high degree of symmetry and a lack of ongoing major merger activity, with only a slight potential for disturbance. The central region is the most intensely illuminated, fading gradually towards the outer edges. The overall shape appears roughly round, though with a small degree of elongation along one axis.
