The galaxy presents a generally smooth, elliptical morphology. It appears to be undergoing a significant merger event. There is a primary, somewhat spheroidal component and a smaller secondary component. The primary component exhibits a smooth, diffuse profile, suggesting a relatively old stellar population. The galaxy presents a yellowish-orange color, indicative of an evolved stellar population, although some bluer tinges may be indicative of an area of star formation. The overall luminosity suggests a massive galaxy. There is a faint halo surrounding the primary and secondary components, possibly indicating a past major merger event. The merger exhibits an estimated size of several kiloparsecs. There appears to be a tidal tail structure emerging from the merging system, though more data would be required to confirm the nature of these potential tidal features. 
