The galaxy exhibits a largely featureless, smooth morphology. It appears elliptical, with a luminosity profile that increases sharply toward the center. The galaxy is nearly symmetrical, displaying only a very slight elongation along one axis. There is little evidence of spiral arms or dust lanes. The core of the galaxy appears very bright and concentrated, suggesting a substantial central bulge. Faint color variations are subtly present, with the central bulge appearing slightly redder than the outer regions. Overall, the galaxy seems to be relatively isolated with no signs of major mergers or tidal disturbances. The light appears relatively uniform, indicative of an older stellar population with a low star formation rate.
