The galaxy appears as a relatively smooth, centrally concentrated object. It has a generally elliptical morphology, exhibiting a somewhat round shape. The galaxy's color profile suggests a lack of substantial recent star formation, as indicated by its redder hue. There is no prominent spiral arm structure or dust lane obscuration visible. Faint, diffuse extensions are observed that are relatively symmetrical, giving it a round appearance. No signs of major ongoing merger activity are apparent, although a possibility of minor disturbances due to tidal interactions cannot be excluded with certainty.
