The galaxy presents as a moderately luminous elliptical, with an apparent redshift. The core region is a concentrated, bright yellowish-white, indicative of an older stellar population. The outer regions diffuse outward, becoming fainter in intensity, and exhibit a slight elongation. The color gradient appears to be relatively smooth, suggesting a lack of significant recent star formation activity across the galaxy. There is the possibility of a minor interaction or disturbance hinted at by the slight asymmetry in the outer halo of the object. The overall morphology appears dominated by a spheroidal component.
