The galaxy exhibits an elliptical morphology, appearing relatively smooth and featureless. The light distribution indicates it is concentrated towards the center, with a gradual decrease in intensity outwards. There is a suggestion of a merging event, possibly with a smaller companion, indicated by the dual concentration of light and a minor disturbance to the main body. The galaxy displays a reddish hue, suggesting an older stellar population, but there might be minimal presence of bluer, younger stars. This galaxy is relatively massive. There is low star formation activity occurring within the galaxy.
