The galaxy presents as a generally smooth, elliptical morphology. It exhibits a bright, concentrated central bulge, with a radial decrease in luminosity outward. The major axis of the galaxy appears significantly longer than the minor axis, suggesting a moderate ellipticity. There is a slight hint of a disk component. The galaxy's color profile appears to be dominated by older stellar populations, as indicated by the yellowish-red hue. There is little evidence of significant dust lanes or active star formation regions within the galaxy. There may be slight evidence of minor disturbances in the outer halo, but no signs of any major ongoing merger events. 
