The galaxy presents an elliptical morphology with a smooth light distribution, characterized by a bright, concentrated central bulge. The light is generally redder towards the central region, indicating an older stellar population. A faint, extended halo surrounds the main body of the galaxy. There is a slight asymmetry observed, possibly indicating a minor disturbance or interaction. Star formation appears to be primarily concentrated in the nuclear region, with little evidence of widespread activity throughout the rest of the galaxy. The overall structure suggests a relatively evolved galaxy, likely a massive elliptical that is undergoing little active merging. 
