The galaxy presents as a compact object, with an apparent circular morphology. The central region displays a pronounced concentration of light. There is a distinct color gradient, shifting from bluer hues towards the core to redder tones in the outer regions of the galaxy's halo. The smoothness of the light distribution suggests a relatively relaxed morphology with no significant, large-scale disturbances visible. Possible irregularities in the light distribution might be present within the innermost region of the galaxy, warranting further investigation to determine the galaxy's type.
