The galaxy appears to be a relatively smooth, elliptical type, with a high degree of central concentration. The core region exhibits a pronounced yellowish hue, possibly indicative of an older stellar population. There is some evidence of faint, extended emission surrounding the central region, characterized by a more greenish color, which may indicate more recent star formation. The overall shape is generally round. No obvious tidal features or signs of major disturbances are discernible. Faint color variations may imply underlying structures.