The galaxy exhibits an overall smooth, elliptical morphology. Its light profile demonstrates a strong central concentration, with a bright, well-defined nucleus transitioning outward to a more diffuse halo. The halo appears relatively uniform, lacking any distinct spiral arm structures or prominent dust lanes. Color gradients are subtle, with a slightly redder core region possibly indicating an older stellar population, gradually fading to a bluer hue in the outer regions, suggestive of a sparse presence of younger, hotter stars. The galaxy's shape is somewhat flattened, displaying an elliptical form. There is no evidence of ongoing major mergers or tidal disruptions; the galaxy appears relatively undisturbed.
