The galaxy presents a predominantly smooth morphology, with a high degree of central concentration. The luminous core transitions into a more diffuse, extended halo. The galaxy exhibits a generally elliptical shape, appearing largely undisturbed. There are very minor indications of a possible disk component; however the overwhelming light from the spheroidal component diminishes that determination. The color profile suggests a population of older stars, with a relatively low rate of star formation, resulting in a redder overall color. There is no apparent major merger event or interaction with another galaxy, although slight distortions suggest minor disturbances.