The galaxy exhibits a complex morphology indicative of an ongoing merger event. Two distinct, roughly elliptical or spheroidal components are visible, each displaying a relatively smooth light distribution. The color profile of each component appears consistent, with a yellowish hue suggesting an older stellar population. There is a small amount of blue color present, indicating some star formation. The tidal features are not very pronounced, suggesting a later stage of merging. There is some indication of minor disturbances but no major disturbance. The luminosity profile suggests this is a very bright and massive object. The overall structure suggests the system is still relatively intact, with the two components maintaining their individual identities to some degree.
