The galaxy presents as a centrally concentrated object with a smooth, somewhat elliptical morphology. A bright, yellowish core is surrounded by a more diffuse, fainter halo or disk. The primary light emission appears to be from older stellar populations, as indicated by the yellow hue. There is a subtle hint of bluer light in the outer regions, suggesting the presence of some younger stars or ongoing star formation, but it is minimal. The galaxy exhibits a relatively undisturbed structure, showing no obvious signs of major mergers or tidal interactions. There might be a very subtle distortion in shape that could imply a minor interaction in the past. The overall appearance suggests this galaxy is most likely a lenticular or early-type spiral galaxy observed at some distance.
