The galaxy appears as a smooth, centrally concentrated object. Its overall morphology is elliptical, with the longer axis roughly twice the length of the shorter axis. There are no readily discernible spiral arms or a well-defined disk structure. The color gradient transitions from a bluish hue in the outer regions to a more reddish-yellow core. This color gradient suggests the presence of older stellar populations in the core compared to potentially younger, bluer stars in the periphery. The galaxy does not show any obvious signs of a recent major merger or significant tidal disturbances. There might be some minor asymmetry or disturbance, but it is minimal.
