The galaxy presents a generally elliptical morphology, appearing mostly smooth with a central, concentrated bulge. The color profile indicates a prominence of older stellar populations, shown by the yellowish-red hue, suggesting a relative lack of ongoing, significant star formation. There is some slight indication of a faint, possibly diffuse, disk-like structure surrounding the central bulge. The object appears to be relatively undisturbed, with only minor possible disturbances. There does not seem to be any active merging events.