The galaxy appears relatively smooth and compact in morphology. The light distribution suggests an elliptical or lenticular galaxy type, lacking prominent spiral arms or a well-defined disk structure. There is a slight elongation, but it is mostly round in shape. The galaxy exhibits a color gradient, appearing somewhat bluer toward the center and redder in the outer regions. The overall color suggests a population of older stars and a low rate of current star formation. There are signs of tidal disturbance or merger activity, indicated by diffuse, low-surface brightness features extending outward from the main body. These features may represent stellar material stripped from the galaxy during past interactions with other galaxies. Overall, the galaxy presents characteristics of a relatively massive, evolved system possibly undergoing or having undergone a merger event.
