The galaxy presents as a relatively smooth, elliptical-like structure. The central region exhibits a high degree of brightness, suggestive of a concentrated stellar population and/or active galactic nucleus. The light appears to shift from yellow-white at the center to faint hues of green as it moves to the outer regions. The ellipticity is moderate; tending towards a spheroid. There is no strong evidence of spiral arm structures or a prominent disk. There are no significant signs of tidal tails or other major disturbances indicative of recent major merger events. Overall, the galaxy appears to be a relatively undisturbed system.
