The galaxy appears to be an elliptical galaxy, characterized by a smooth, spheroidal morphology. It exhibits a concentrated central region, suggesting a high stellar density. The color profile indicates an older stellar population, with a yellowish-orange hue dominating the galaxy's light. There is little evidence of spiral arms or dust lanes. The overall structure is relatively undisturbed, showing no prominent signs of recent major mergers or tidal interactions. The galaxy's luminosity suggests it is a massive system. There may be some ongoing star formation but at a low rate.
