The galaxy appears as a centrally concentrated, relatively smooth object. It possesses a roughly elliptical morphology, exhibiting a slight elongation without exhibiting characteristics of a spiral structure. The galaxy displays a consistent color profile with only small variations, indicating a lack of prominent star-forming regions. The overall color index suggests a moderately evolved stellar population. There is no evidence of a strong tidal interaction or ongoing merger. The light distribution gradually fades toward the outer regions, demonstrating a well-defined boundary.
