The galaxy presents an elliptical morphology, elongated along a primary axis. Its core exhibits a bright, yellowish-white hue, indicating a concentration of older stellar populations. This central region gradually fades into a more diffuse, bluish halo. The presence of blue suggests the existence of some younger stars or regions of ongoing star formation. A faint extension emanates from one side of the galaxy, possibly a tidal feature or a minor disturbance suggesting a past interaction. The overall structure appears relatively smooth, with a substantial fraction of light coming from a featureless component, with some disk-like characteristics. The color gradients imply variations in stellar populations or dust content across the galaxy.
