The galaxy presents as a relatively smooth, centrally concentrated object, exhibiting a near-spherical morphology. Its light profile appears dominated by an elliptical distribution, lacking any discernible spiral arm structures or prominent dust lanes. The core region displays a bright, yellowish hue, indicative of an older stellar population potentially abundant in red giant stars. The outer regions of the galaxy exhibit a more diffuse, reddish-orange coloration, suggesting a presence of evolved stars. There are no clear signs of recent major mergers or tidal disturbances, though a very faint, asymmetric extension on one side suggests a potential interaction with a smaller companion, but it is also likely an artifact. Overall, the galaxy gives the impression of a fairly evolved system with relatively low levels of ongoing star formation.
