The galaxy presents a generally smooth, elliptical morphology. It exhibits a radial concentration of light, with the brightest region centrally located, suggesting a prominent galactic nucleus. The overall shape is mostly round. Subtle variations in color are visible, with a slightly reddish hue dominating the central region, potentially indicating an older stellar population. Fainter, bluer regions are present in the outer regions, possibly indicative of ongoing or recent star formation. There does not appear to be any indication of a major merger event, such as tidal tails or significant morphological distortions. A slight asymmetry may be present in the outer halo.
