The galaxy presents an elliptical morphology, appearing largely smooth and featureless. It exhibits a concentrated central bulge with a gradual decrease in luminosity towards its outer regions. The galaxy's overall color profile suggests a predominantly older stellar population, with a yellow-red hue indicative of evolved stars. There is no evidence of prominent spiral arms or dust lanes within the visible spectrum. The shape of the galaxy is neither perfectly round nor elongated, but somewhere in between. There are no obvious signs of a major ongoing merger, though some minor disturbances cannot be ruled out.
