The galaxy presents an elliptical morphology, elongated along its major axis. It exhibits a smooth light distribution, lacking prominent spiral arms or distinct features suggestive of ongoing major mergers. There may be a very slight warping in the disk. The central region displays a concentration of light, indicating a bulge component, with color suggesting an older stellar population that might have little star formation. The outer regions appear more diffuse, with a subtle color gradient, possibly indicating an aging population in the halo. The galaxy shows no evidence of strong tidal interactions or recent merging events, appearing relatively isolated and undisturbed. There are hints of minor disturbances in the disc.
