The galaxy appears to be an elliptical galaxy, exhibiting a smooth, featureless morphology. It presents with a concentrated central bulge that gradually fades into the outer regions. There is no apparent spiral arm structure or dust lane. The galaxy has a slight golden hue, likely resulting from an older stellar population, with the majority of star formation already completed. The overall shape is roughly elliptical, leaning towards being in between round and elongated, with minimal signs of recent or ongoing merger activity. The light is centrally concentrated, suggesting a relatively relaxed dynamical state. There are no obvious tidal tails or distortions.
