The galaxy appears as a relatively smooth, elliptical-like structure. The core region exhibits a bright, concentrated luminosity, suggesting a high density of stars. The color gradient transitions from a bluish-white central region to a more reddish hue in the outer areas of the galaxy, which might indicate younger stars. The galaxy displays no visible spiral arm structure or prominent dust lanes. There is a slight suggestion of a disk-like shape. There is little evidence of any significant ongoing merger activity or major disturbances in its morphology, but there might be some subtle signs of a minor disturbance, like a small asymmetry or irregularity in the halo. 
