The galaxy presents as a centrally concentrated, elliptical-like structure. The core exhibits a bright, yellowish-white luminosity, suggesting a population of older stars. A relatively smooth light distribution is observed, indicating a lack of prominent spiral arms or significant dust lanes. The overall shape is nearly circular, displaying minimal elongation. There is a subtle color gradient, with the central region appearing slightly redder than the outer halo. The galaxy's profile suggests minimal interaction or disturbance from neighboring galaxies. Evidence of recent or ongoing major mergers are not apparent in the images, only a slight minor disturbance can not be ruled out.
