The galaxy presents as an elliptical morphology, appearing smooth and largely featureless. It exhibits a concentrated central bulge, which dominates the overall light profile. The light gradually diminishes towards the outer edges of the galaxy. The galaxy displays a yellow-red hue, suggestive of an older stellar population. There's no obvious dust lane, spiral arm structure, or active star-forming regions visible. The isophotes appear generally round. There is no obvious visual evidence of any major merger events. The galaxy may be experiencing minor gravitational disturbances.
