The galaxy presents as a relatively smooth, elliptical-like structure. Its light is concentrated in the center, forming a bright, yellowish core. The outer regions of the galaxy appear fainter, with a gradual decrease in surface brightness towards the edges. The overall color profile indicates a population of older stars, particularly in the central bulge, with potentially some younger, bluer stars mixed in the outer regions. There is no clear evidence of spiral arms or a well-defined disk. The galaxy appears mostly undisturbed, without any major signs of ongoing mergers or tidal interactions, though subtle irregularities could indicate a minor past interaction. The shape is somewhat elongated but generally rounded.
