The galaxy presents a complex morphology, suggesting an ongoing or recent interaction/merger event. The primary body of the galaxy appears relatively smooth and elliptical in shape, exhibiting a concentrated central bulge that fades out into a more diffuse halo. There is a secondary component which is less luminous, but it is not clear whether it is another galaxy interacting with the main component, or a star forming region within the galaxy that is separate from the primary central bulge. The tidal distortions and asymmetric light distribution hints at gravitational disturbances. The overall color suggests a mix of stellar populations, the primary component has a yellowish color with hints of bluer stars at the outer edges. The secondary component appears to have bluer color, possibly indicating an elevated rate of star formation.
