The galaxy presents as a largely featureless, elliptical morphology. Its overall form is smoothly distributed with a high degree of central concentration. The color gradient transitions from a brighter, yellowish core region to a redder, more diffuse outer halo. There is no evidence of spiral arms, a prominent disk, or ongoing major merger activity. Minor irregularities in the outer regions suggest possible past interactions or minor disturbances. It has a roughly circular appearance in the image, indicating it may be close to face-on orientation with respect to the observer. The galaxy exhibits low levels of star formation activity.
