The galaxy presents an overall elliptical morphology. The central region exhibits a bright, concentrated core suggesting a significant population of older stars. Proceeding outward from the core, the brightness diminishes, with the galaxy's outer regions appearing more diffuse. The color profile appears redder in the core and shifts towards bluer hues further from the center, indicating the likely presence of younger stellar populations in the outer regions. There appears to be some form of disturbance that indicates this galaxy may be undergoing or recently underwent a merger. The axial ratio indicates a relatively flattened shape.
