The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a generally elliptical morphology, appearing largely spheroidal in shape with a high degree of circularity. There is no clear evidence of spiral arms, bars, or significant dust lanes. The light distribution suggests a dominant bulge component, possibly indicating an older stellar population. The galaxy appears to be relatively undisturbed, showing no obvious signs of a major ongoing merger or tidal interactions, though subtle asymmetries may hint at minor disturbances. Color gradients are present, with a bluer hue towards the outer regions compared to the whiter, brighter central core.
