The galaxy presents as a slightly elongated, lenticular structure. The central bulge region exhibits a bright, yellowish-white hue, suggesting a concentration of older stellar populations. Progressing outwards, a fainter, bluer disk is observed, indicating the presence of ongoing, although subdued, star formation. The edges of the disk appear relatively smooth, lacking prominent spiral arm structures or significant dust lanes. There are no obvious signs of major tidal disturbances or ongoing mergers, although a slight asymmetry in the outer disk might suggest a past interaction or minor disturbance. Overall, the galaxy has a relatively featureless appearance, with a smooth luminosity gradient from the central bulge to the outer regions.
