The galaxy presents as a concentrated elliptical morphology. It exhibits a generally smooth, symmetrical light distribution, with a noticeable lack of spiral arm structure. The core is bright and concentrated, and the galaxy appears more rounded than elongated. There's a slight suggestion of some minor structural disturbances, potentially related to a past interaction or merger, but there is no significant distortion of the overall shape and it appears mostly undisturbed. The galaxy exhibits a yellow/red hue, indicating an older stellar population, and a likely low star formation rate. Its mass appears substantial.
