The galaxy appears to be a relatively smooth, elliptical system. It exhibits a high degree of circularity, with a slight elongation. The galaxy's light profile suggests a concentrated bulge. Little evidence of distinct spiral arms or prominent disk structures are apparent. The core region appears luminous, possibly indicating the presence of an active galactic nucleus or a dense concentration of stars. The overall color is yellowish-red, suggesting a relatively old stellar population with diminished active star formation. There is no obvious sign of significant tidal disturbances or ongoing major merger activity. Minor disturbances or past merger events can not be ruled out. 
