The galaxy presents as an elliptical morphology, appearing generally smooth and well-rounded in form. There is a bright, concentrated central bulge that gradually diffuses into a fainter, extended halo. No prominent spiral arms or significant disk-like structures are readily apparent. The overall color is yellowish-orange, suggesting a population of older stars and a relatively low rate of on-going star formation. There are no obvious signs of recent major merger activity or tidal disturbances. Based on its color and morphology, the galaxy is likely a relatively massive system.
