The galaxy exhibits an elliptical morphology, with a largely smooth, centrally concentrated light distribution. The primary color is a yellow-white hue, suggesting a stellar population that is dominated by older, evolved stars. There may be evidence of a minor interaction or disturbance on one side of the central region, appearing as a redder region, potentially indicating a region of ongoing or recent star formation. The galaxy is relatively compact in apparent size. The roundness appears somewhere in between perfectly round and slightly elongated. There is no sign of any major ongoing merger, but possible signs of minor disturbances. The galaxy appears relatively massive given the color.
