The galaxy appears as a singular, relatively smooth object with a generally round morphology. There is little evidence of spiral arm structure or significant dust lanes within the visible light spectrum. The galaxy exhibits a concentrated light profile, potentially indicative of an elliptical galaxy or a lenticular galaxy seen face-on. The color is predominantly reddish-yellow, suggesting an older stellar population and suppressed recent star formation activity. There is no clear visual indication of a major ongoing merger, but the possibility of minor tidal disturbances cannot be completely ruled out. The galaxy's overall appearance aligns with a well-evolved system approaching quiescence.
