This galaxy exhibits an elliptical morphology with a smooth light distribution. It appears to be a relatively massive galaxy, possibly with a supermassive black hole at its center. The light is concentrated towards the core, with a distinct yellow/orange hue, suggesting an older stellar population and a low star formation rate. This color also indicates the presence of a significant population of red giant stars. It is slightly elongated, and there might be a minor tidal disturbance, but this galaxy does not appear to be in the midst of a major merger. The lack of defined spiral arms or dust lanes further supports its classification as an elliptical galaxy.
