The galaxy appears as a centrally concentrated object with a generally smooth morphology. It exhibits a bright central bulge that dominates the overall luminosity. The elliptical shape is discernable, showing a slight flattening and indicating a degree of rotational support. Color gradients within the galaxy suggest a stellar population that is redder and likely older towards the core, with a gradual bluing towards the outer regions, hinting at some recent star formation in the outer disk or halo. The galaxy does not appear to show any prominent spiral arm structure or major disturbances, indicating it is most likely undisturbed. It is fairly compact, with a clearly defined edge.
