The galaxy presents as a relatively smooth, elliptical-like structure with a concentration of light towards the center. The core region exhibits a yellowish hue, suggestive of an older stellar population. There is a secondary, less defined region of diffuse light, slightly offset from the main body, appearing more bluish-white. This could indicate a region of more recent star formation, possibly the remnant of a tidal interaction or an ongoing minor merger event. The overall morphology hints at a system undergoing, or having recently undergone, some form of dynamical disturbance. A significant fraction of the galaxy's light is concentrated in the core, while the outer regions are comparatively faint.
