The galaxy presents a largely elliptical morphology, exhibiting a smooth, featureless appearance. Its color profile suggests a dominant population of older stars, inferred from the redder hues observed in the outer regions. The galaxy appears relatively undisturbed, lacking any significant signs of tidal interactions or ongoing merger events. The luminosity profile indicates a centrally concentrated structure, with a gradual decline in brightness towards the periphery. Its relatively small angular size is consistent with it being a more distant object. Based on the light profile, it is likely an elliptical galaxy.
