The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The light distribution appears consistent with an early-type galaxy. The color profile suggests a dominant population of older stars, as evidenced by the yellowish-red hue. There's no discernible spiral structure or dust lanes visible. The galaxy appears fairly isolated, with no obvious signs of major ongoing mergers, although some minor asymmetry might indicate a past interaction or minor disturbance. Overall, the galaxy exhibits a high degree of radial symmetry and uniform light distribution.
