The galaxy presents as a luminous, centrally concentrated object. It exhibits a smooth, elliptical morphology with a high degree of symmetry. The galaxy's light profile appears to decrease gradually from the bright core, lacking any distinct spiral arm structures or prominent dust lanes. There is no distinct disk component. Color gradients are subtle, with a slightly bluer hue in the outer regions compared to the more reddish central bulge. This suggests a potentially older stellar population dominating the core, with some ongoing star formation activity towards the outskirts. The object shows a notable ellipticity, deviating somewhat from a perfect circular shape. There are no obvious signs of tidal disturbances or major mergers visible in this image, indicating a relatively quiescent state.
