The galaxy presents a generally smooth and centrally concentrated morphology. It appears elliptical in shape, with a noticeable elongation along one axis, though it is not extremely flattened. The central region displays a bright, concentrated core that fades gradually into the outer regions. No distinct spiral arm structures are apparent. The light distribution suggests a relatively uniform stellar population, lacking prominent dust lanes or regions of intense star formation activity. There are no obvious signs of ongoing or recent major merger events, although a slight asymmetry or minor disturbance cannot be entirely ruled out. The overall color is relatively red, indicating an older stellar population, consistent with a low specific star formation rate.
