The galaxy presents an elliptical morphology, exhibiting a smooth and diffuse light distribution. The central region displays a notably high surface brightness, gradually decreasing towards the outer edges. There is a slight flattening observed, suggesting it is not perfectly spherical. No distinct spiral arms or bar structures are discernible in the image. The overall color appears slightly redder than the surroundings, possibly indicating an older stellar population and/or dust content. There are no obvious signs of ongoing major merger activity or significant tidal disturbances, although a subtle asymmetry in the outer halo cannot be excluded with the available data.
