The galaxy presents as an elliptical morphology, with a smooth and featureless appearance. It exhibits a centrally concentrated luminosity profile, suggesting a significant bulge component. The galaxy's color gradient transitions from a yellowish-orange core to a bluer halo. The overall shape appears elongated, with a moderate ellipticity. There is no discernible evidence of spiral arms or active star formation regions within the visible spectrum. The galaxy appears to be isolated, lacking any signs of recent or ongoing mergers or tidal disturbances.
