The galaxy presents as an elliptical morphology with a smooth, concentrated light profile. The core region exhibits a yellowish-white hue, suggestive of an older stellar population and potentially lower levels of ongoing star formation. The outer regions of the galaxy appear to be less defined with a more irregular edge, and there is a subtle blue color gradient indicating the presence of younger stars. The galaxy appears undisturbed, without any signs of major merging or tidal features. Faint, diffuse extensions of light are observed beyond the core, possibly indicating a halo of older stars.
