The galaxy appears as a relatively smooth, elliptical object with a concentrated central bulge. The overall color profile suggests an older stellar population, exhibiting a yellowish hue, with the potential for a subtle redder component in the core region. There is little evidence of active star formation. The galaxy's shape is more rounded than elongated. There is no obvious indication of a major merger event, although a minor disturbance cannot be completely ruled out due to the faint and somewhat irregular outer structure. There is a secondary light structure near the central bulge that could indicate recent interaction or merging.
