The galaxy presents as a somewhat compact object with an apparent disturbance in its morphology. The primary structure appears elliptical in form, with a concentration of luminosity toward the center. There is a distinct secondary, less luminous component that appears to be interacting gravitationally with the primary component. This could be the result of an ongoing or recent merger event, resulting in the disturbed morphology observed. The colour distribution shows the primary component is brighter in red wavelengths than the secondary component, and the secondary component appears brighter in bluer wavelengths. This suggests the primary component is likely more evolved with a higher population of older stars, and the secondary component is an area where active star formation is occurring. There is also a blue clump separate from the other bodies in the image which seems to be related to the merger that is occurring.
