The galaxy appears to be an elliptical galaxy, exhibiting a smooth, symmetrical morphology. It presents a concentrated central bulge region that gradually fades into an extended halo. The light distribution suggests an older stellar population, as indicated by its reddish hue. There is no discernible dust lane or spiral arm structure, further supporting its classification as an elliptical galaxy. The overall round shape is characteristic of galaxies of this type. No signs of recent or ongoing merger activity are readily apparent in this image.
