The galaxy presents as a centrally concentrated, relatively smooth, elliptical morphology. There appears to be a distinct bulge component. Color gradients suggest an older stellar population dominating the central regions, evidenced by the redder hue. A less pronounced but still observable, bluer component extends outwards from the core, indicating a younger stellar population. There is no readily apparent evidence of spiral arm structure or significant dust lanes. The overall appearance is consistent with a galaxy that has undergone significant evolution and is currently exhibiting a relatively low star formation rate. The galaxy does not exhibit obvious signs of a major merger event, though there could be evidence of minor tidal disturbance.
