This galaxy exhibits a centrally concentrated light profile, typical of an elliptical galaxy. The core is bright and smoothly blends outwards, with no apparent spiral arm structure or dust lanes. It appears slightly elongated, suggesting a non-spherical shape. The color appears somewhat red, possibly indicative of an older stellar population and reduced star formation. The galaxy is relatively compact. There may be evidence of a slight disturbance. Overall, the galaxy appears as a relaxed, relatively evolved system.
