The galaxy presents a generally smooth and elliptical morphology. It exhibits a concentrated central bulge, gradually fading into an extended halo. The light distribution suggests a relatively high degree of symmetry. There appears to be a slight flattening, moving away from a perfectly circular profile. The color index indicates a population of evolved stars, possibly indicating a relatively low rate of on-going star formation, with the central region appearing bluer than the outer regions. There is no apparent sign of any major merger events, tidal tails, or other major disturbances. A minor asymmetry may be present in the outer halo.
