The galaxy appears as a luminous, elliptical structure. It exhibits a smooth and concentrated central bulge, with a gradual decrease in luminosity towards its outer regions. The overall color profile suggests a relatively evolved stellar population, leaning towards older, redder stars. There is little indication of prominent spiral arms or active star formation regions within the observed bands. The galaxy's shape is moderately elongated, appearing more disc-like than spherical. No significant tidal features or signs of ongoing major mergers are clearly visible, though a slight asymmetry in the outer regions suggests a possible minor interaction or disturbance. 
