The galaxy presents as a relatively smooth, elliptical-like structure. The central region displays a concentrated, bright yellowish-orange hue, suggestive of an older stellar population. The outer regions exhibit a gradual fading of luminosity, trending towards a more diffuse and slightly bluer appearance. There is no clear evidence of spiral arms or significant dust lanes, which supports its classification as likely an elliptical galaxy. The overall form is somewhat rounded but not perfectly spherical. There is no clear indication of any major mergers occurring. Minor disturbances may be present, but are not easily discernible. The color suggests ongoing but subdued star formation activity within the galaxy.
