The observed galaxy presents as a generally smooth, elliptical structure with a concentrated central bulge. The core exhibits a notably bright, yellowish hue indicative of a population of older stars. The light gradually diffuses outward from the core into a less defined halo. Faint blue edges indicate the presence of some younger stars towards the edge of the galaxy, but their presence is not as dominant as the overall yellow color. There is no clear evidence of defined spiral arms or significant dust lanes. The overall shape is somewhat round, appearing neither significantly elongated nor disturbed. There does not appear to be any indication of major mergers or tidal distortions. The galaxy's extended halo is subtle and fades into the background sky without any distinct edge.
