The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge, characterized by a bright, yellowish-white hue, suggesting a population of older, less active stars. The outer regions of the galaxy display a fainter, slightly bluer color, possibly indicating the presence of younger stars or ongoing star formation, however it is also possible that the blue shift is from it being further away. There are no obvious signs of spiral arms or a distinct disk component. The overall shape appears somewhat elongated, tending towards a more spherical form, but not perfectly round. There is no indication of significant tidal disturbances or merging activity, suggesting that the galaxy is currently in a relatively quiescent state. The galaxy appears to be relatively undisturbed and isolated in its environment.
