The galaxy appears as a relatively smooth, centrally concentrated object with a slightly elongated morphology. The light profile suggests a dominant bulge component, with a gradual decrease in intensity outward. There is no clear evidence of spiral arm structure or prominent dust lanes within the galaxy's disk, further supporting a classification as a smooth galaxy type. A subtle color gradient is apparent, shifting from a slightly bluer hue towards the outer regions. Based on this information, the galaxy is plausibly an elliptical or S0 galaxy. There are no signs of active galactic nuclei features such as tidal tails or distortions.
