The galaxy presents as a somewhat smooth, elliptical object. It exhibits a concentrated central bulge that appears yellowish, possibly indicating an older stellar population. The outer regions of the galaxy show a more diffuse, bluish hue suggesting the presence of some younger stars, although the overall color suggests a more evolved system. The shape is neither perfectly round nor highly elongated, presenting an in-between profile. There might be some minor disturbances visible, potentially indicative of a past or ongoing minor interaction or internal dynamic processes. However, a major merger event seems unlikely due to the generally undisturbed structure. There may also be some amount of star formation occuring in the galaxy, though most likely at a lower rate than more active spiral galaxies.