The galaxy presents as a centrally concentrated elliptical morphology, appearing largely featureless in this image. It exhibits a smooth luminosity profile, with the brightest region located at the core and a gradual decrease in surface brightness moving outwards. The core region shows a yellow to slightly orange hue, suggestive of an older stellar population. The outer regions exhibit a slightly bluer tint, though the image resolution limits our ability to resolve any distinct spiral arms or star-forming regions. The overall shape is somewhat elongated but very close to round. No signs of tidal disturbances, mergers, or active galactic nuclei are readily apparent.
