The galaxy presents as a roughly elliptical, though somewhat elongated, structure. A dominant yellowish hue characterizes the central region, suggestive of an older stellar population. Fainter, diffuse, and slightly bluer extensions emanate from the central region; these may indicate the presence of recent star formation activity. The galaxy does not appear perfectly smooth; there is a faint hint of asymmetry or a possible minor tidal disturbance visible on one side, potentially indicating an ongoing interaction or merger event. There may be hints of very faint tidal tails, though the signal is weak.
