The galaxy presents as an elliptical or lenticular type, appearing largely smooth with a concentrated central bulge. It exhibits a subtle elongation, deviating slightly from a perfectly spherical shape. Coloration is primarily concentrated in the central region, trending towards bluer wavelengths with a subtle shift toward redder hues in the outer regions. There is no indication of strong spiral arm structure or prominent dust lanes within the galaxy. No apparent ongoing major merger events are observed, and only minor disturbances or tidal features could be present, but are difficult to confirm.
