The galaxy presents an elliptical morphology, exhibiting a smooth, diffuse light distribution with a highly concentrated central bulge. The galaxy's color profile appears to shift from a yellowish-white core to a bluer halo, suggesting a change in stellar population with radius, possibly indicating that the central bulge contains older, redder stars, and a halo with younger bluer stars. The galaxy's shape has some elongation. There is no apparent disk structure. The image reveals no obvious signs of recent major merger activity, nor any prominent tidal tails or shell structures. Given the observed features, the galaxy is likely an early-type galaxy, possibly an elliptical galaxy undergoing a very low rate of star formation.
