The galaxy presents as a largely featureless, elliptical-like object with a smooth, concentrated light distribution. The central region exhibits a bright, yellowish-white hue, suggesting a population of older stars. A subtle color gradient appears to exist with the outer regions transitioning to a dimmer, slightly redder shade, possibly indicative of older stellar populations and/or dust obscuration. There are no apparent spiral arms or dust lanes visible. The overall shape is close to circular with no signs of major tidal disturbances or ongoing mergers.
