The galaxy presents a smooth, elliptical morphology. The light is concentrated towards the center, displaying a bright central bulge. There's a general lack of distinct spiral arms or substructure. The galaxy appears relatively isolated, showing no signs of major mergers or significant tidal disturbances. Its overall color profile suggests an older stellar population, with a redder hue dominating. There might be only minor or no current star forming regions, since the color is not as blue as galaxies with active star formation. It appears to have a disk-like shape, but it is hard to determine the roundness from the image alone.
