The galaxy presents an elliptical morphology with a smooth, diffuse light distribution. The central region exhibits a pronounced concentration of luminosity, suggesting a significant stellar density and likely a supermassive black hole at its core. Moving outward, the galaxy's luminosity gradually diminishes, transitioning into a fainter, more extended halo. While a subtle disc-like structure may be present, there are no spiral arms or distinct features indicative of active star formation readily visible in this image. A slight asymmetry in the outer halo suggests a minor gravitational interaction or past merger event; a minor disturbance is suggested in the overall structure of the galaxy. The overall color is reddish, indicating an older stellar population with less ongoing star formation, consistent with an elliptical classification. The object appears moderately distant.
