The galaxy appears as a centrally concentrated object, exhibiting a smooth, elliptical morphology. It possesses a bright, well-defined core region that gradually decreases in intensity outwards. The color profile is predominantly reddish-yellow, suggesting a stellar population dominated by older, evolved stars. There is no obvious evidence of spiral arm structures or significant dust lanes within the visible light spectrum. The overall shape is generally rounded with a slight elongation and lacks any indications of major merger events or tidal distortions. Minor asymmetry in the outer regions may indicate past interactions, however they are not obvious in the image. Overall it appears to be a fairly relaxed and relatively quiescent system.
