The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge with a gradual decrease in luminosity extending outwards. The primary color appears to be a yellowish-orange, indicative of an older stellar population and limited current star formation. There may be some minor irregularities present in the outer regions of the galaxy, but the dominant impression is one of relative symmetry and established structure. It does not appear to be undergoing any major merger events, although subtle disturbances may be present.
