The galaxy presents as a relatively smooth, concentrated object. It appears elliptical in shape, with a notable absence of distinct spiral arm structures. The primary light emission seems to originate from an older stellar population, indicated by the redder hue concentrated near the center. However, there is also a small region which appears blue in color indicating a younger population of stars. The galaxy appears to be relatively isolated, with no immediately apparent signs of a major ongoing merger, though some minor tidal disturbance cannot be ruled out based on the morphology alone. There is a slight elongation or possible tidal feature visible on the left side of the galaxy. The overall color suggests moderate star formation. The galaxy exhibits a somewhat round shape.
